8867( 21) - 12/14/01 17:23 - [ 1] PROPOSAL FOR HUBBLE SPACE TELESCOPE OBSERVATIONS ST ScI Use Only ID: 8867 Version: 21 Check-in Date: 14-Dec-2001 17:18:40 1.Proposal Title: Gamma-ray bursts: discovering the progenitors and understanding the explosion - visits A0-R0 ------------------------------------------------------------------------------------ 2. Proposal For 3. Cycle GO 9 ------------------------------------------------------------------------------------ 4. Investigators Contact? PI: Shrinivas Kulkarni California Institute of Technology CoI: Dr. T. Axelrod Mt. Stromlo Observatory N CoI: Dr. B. Schmidt Mt. Stromlo Observatory N CoI: Dr. R. Kimble Goddard Space Flight Center N CoI: Dr. J. Holtzman New Mexico State University N CoI: Dr. H. Marshall Massachusetts Institute of Technology N CoI: Prof. R. Chevalier University of Virginia N CoI: Dr. T. Murakami Institute for Space Astronautics and N Sciences CoI: Dr. F. Frontera Ist. Tecn. Studio delle Rad. N Extraterrestri CoI: Dr. E. Costa Ist. di Astrofisica Spaziale N CoI: Dr. L. Piro Ist. di Astrofisica Spaziale N CoI: Dr. G. Ricker Massachusetts Institute of Technology N CoI: Prof. C. Wheeler University of Texas N CoI: Dr. A. Diercks California Institute of Technology N CoI: Prof. S. G. Djorgovski California Institute of Technology N CoI: Dr. T. Galama California Institute of Technology N CoI: Prof. F. A. Harrison California Institute of Technology N CoI: Dr. R. Sari California Institute of Technology N CoI: Prof. R. Ellis California Institute of Technology N CoI: Mr. J. S. Bloom California Institute of Technology N CoI: Dr. D. Frail National Radio Astronomy Observatory N CoI: Prof. J. Halpern Columbia University N CoI: Dr. P. McCarthy Obs. of the Carnegie Inst. of Washington N 8867( 21) - 12/14/01 17:23 - [ 2] ------------------------------------------------------------------------------------ 5. Abstract Gamma-ray burst astronomy, one of the most active and exciting frontiers in astrophysics, is now entering a critical stage -- with dramatic leaps in our understanding of these events, as well as new discoveries imminent. In the upcoming year, improvements in triggering and positioning accuracy provided by the SAX and HETE-2 gamma-ray satellites will allow entirely new classes of events to be studied. Given the recent progress in this field, we are now in a position to design precision, broadband measurements that can provide quantitative information on the as-yet unknown energy sources, the explosion geometry, and the surrounding medium. In particular, the growing evidence of an intimate connection between SNe and GRBs can be definitively tested. Who can activate the proposal: Shri Kulkarni srk@astro.caltech.edu Work: (626) 395-4010 Mobile: (626) 676-4721 Home: (626) 795- 7894 Alan Diercks ad@astro.caltech.edu Work: (626) 395-4970 Mobile (626) 676-4724 Home: (626) 577-7390 Titus Galama tjg@astro.caltech.edu Work: (626) 395-8495 Mobile (626) 676-4723 Home: (626) 568-3937-The STIS CCD imaging should occur as quickly as possible after activiation. (visits 1-72.)-The UV sepctroscopy (Visits UW and UV) should begin 2-3 days after activation.-The STIS UV imaging should occur approximately (A0, C0, E0, G0, I0, K0, M0, O0, Q0) 1 week after activation. and goes with The WFPC2 imaging (A1-B0, C1-D0, E1-F0, G1-H0, I1-J0, K1-L0, M1-N0, O1-P0, Q1- R0) should start 15-20 daysafter activation depending on redshfit. ------------------------------------------------------------------------------------ Observations Description ------------------------ We propose a set of HST TOO and standard observations, synergistic with ground- based radio, IR and optical observations, as well as CXO measurements, designed to answer the outstanding and fundamental questions in GRB astronomy. We believe this program will dramatically alter our understanding of these events, and will become a significant part of the scientific legacy of HST. Real Time Justification ----------------------- Calibration Justification ------------------------- Additional Comments ------------------- ------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 3] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 1 GRB000926 EXT-STAR, GAMMA RAY RA=17H 4M 9.7S +/- 0.2", DEC=51D J2000 R = 19.9+/-0.2 BURSTER 47' 10.0" +/- 0.2", PLATE- ID=00T5 Coordinate Source: IMAGE_TIED_TO_GSC_FRAME 2 GRB010222 EXT-STAR, GAMMA RAY RA=14H 52M 12.55S +/- 0.2", J2000 R = 20.0+/-1.0 BURSTER DEC=43D 1' 6.2" +/- 0.2" Coordinate Source: IMAGE_TIED_TO_GSC_FRAME 3 GRB000630 EXT-STAR RA=14H 47M 13.485S +/- 0.3", J2000 R = 26.0+/-1.0 DEC=41D 13' 53.25" +/- 0.3" Coordinate Source: IMAGE_TIED_TO_GSC_FRAME 4 GRB011211 EXT-STAR, GAMMA RAY RA=11H 15M 17.98S +/- 0.25", J2000 Z = 2.14 R = 21+/-0.5 BURSTER DEC=-21D 56' 56.2" +/- 0.25" Coordinate Source: IMAGE_TIED_TO_GSC_FRAME Comments: Goal is to get offset position, good light curve, and the host galaxy of this moderately-high redshift burst 21 GRB010921 EXT-STAR, GAMMA RAY RA=22H 55M 59.90S +/- 0.6", J2000 R = 21.7+/-0.2 BURSTER DEC=40D 55' 52.87" +/- 0.6" Coordinate Source: OTHER_SOURCE 170 GRB970828 EXT-STAR, GAMMA RAY RA=18H 8M 31.62S +/- 0.25", J2000 R = 24.5 BURSTER DEC=59D 18' 51.32" +/- 0.25" Coordinate Source: OTHER_SOURCE 180 GRB000131 EXT-STAR, GAMMA RAY RA=6H 13M 31.08S +/- 0.25", DEC= J2000 R = 27 BURSTER -51D 56' 41.70" +/- 0.25" Coordinate Source: OTHER_SOURCE 8867( 21) - 12/14/01 17:23 - [ 4] TARGET LIST Generic Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Selection Criteria | Flux data No | Name | Description | | ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-3- EXT-STAR, GAMMA RAY TARGETS=10 V = 24.0+/-1.0 Z0.5 BURSTER, SUPERNOVA, E(V-R) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at z<=0.5 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-3- EXT-STAR, GAMMA RAY TARGETS=20 V = 24.0+/-1.0 0.5Z0.9 BURSTER, SUPERNOVA, E(B-V) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at 0.5<=z<=0.9 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4- EXT-STAR, GAMMA RAY TARGETS=40 V = 24.0+/-1.0 Z0.5 BURSTER, SUPERNOVA, E(V-R) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at z<=0.5 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB-TOO-4- EXT-STAR, GAMMA RAY TARGETS=50 V = 24.0+/-1.0 0.5Z0.9 BURSTER, SUPERNOVA, E(B-V) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at 0.5<=z<=0.9 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 60 GRB-TOO-4- EXT-STAR, GAMMA RAY TARGETS=60 V = 24.0+/-1.0 DUST BURSTER, SUPERNOVA, E(V-R) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at z<=0.5 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 5] TARGET LIST Generic Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Selection Criteria | Flux data No | Name | Description | | ------------------------------------------------------------------------------------------------------------------------------------ 70 GRB-TOO-5- EXT-STAR, GAMMA RAY TARGETS=70 V = 24.0+/-1.0 Z0.5 BURSTER, SUPERNOVA, E(V-R) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at z<=0.5 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 80 GRB-TOO-5- EXT-STAR, GAMMA RAY TARGETS=80 V = 24.0+/-1.0 0.5Z0.9 BURSTER, SUPERNOVA, E(B-V) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at 0.5<=z<=0.9 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 90 GRB-TOO-5- EXT-STAR, GAMMA RAY TARGETS=90 V = 24.0+/-1.0 DUST BURSTER, SUPERNOVA, E(V-R) = 0.5+/-0.15 GALAXY, HIGH REDSHIFT Comments: This TOO consists of broad-band filter WFPC imaging of a GRB at z<=0.5 The mag is an estimate of the mag of the SN component (a point source). In addition there may be some flux from an underlying host galaxy and from the emission from the relativistic blast wave. ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 6] Patterns ------------------------------------------------------------------------------------------------------------------------------------ Pattern_Number: 10 Primary_Pattern Secondary_Pattern Pattern_Type WFPC2-LINE Pattern_Purpose DITHER Number_Of_Points 2 Point_Spacing 0.3535 Coordinate_Frame POS-TARG Pattern_Orient 45 Center_Pattern NO ------------------------------------------------------------------------------------------------------------------------------------ Pattern_Number: 20 Primary_Pattern Secondary_Pattern Pattern_Type WFPC2-BOX Pattern_Purpose DITHER Number_Of_Points 4 Point_Spacing 0.559017 Coordinate_Frame POS-TARG Pattern_Orient 26.565051 Center_Pattern NO ------------------------------------------------------------------------------------------------------------------------------------ Pattern_Number: 60 Primary_Pattern Secondary_Pattern Pattern_Type STIS-CCD-BOX Pattern_Purpose DITHER Number_Of_Points 4 Point_Spacing 0.2835 Coordinate_Frame POS-TARG Pattern_Orient 26.6 Center_Pattern NO ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 7] Visit: 01 Visit Priority: Visit Requirements: SEQ 01, 02, 03 WITHIN 3 D SCHED 100% On Hold Comments: Additional Comments: Visits 01, 02 and 03 together form the study of a GRB host in the 450, 606 and 814 filters. Each filter is observed for 4 orbits each. We here use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB970828 WFPC2 IMAGE WF3 F450W 1 2200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 8] Visit: 02 Visit Priority: Visit Requirements: SCHED 100% On Hold Comments: Additional Comments: Visits 01, 02 and 03 together form the study of a GRB host in the 450, 606 and 814 filters. Each filter is observed for 4 orbits each. We here use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB970828 WFPC2 IMAGE WF3 F606W 1 2200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 9] Visit: 03 Visit Priority: Visit Requirements: SCHED 100% On Hold Comments: Additional Comments: Visits 01, 02 and 03 together form the study of a GRB host in the 450, 606 and 814 filters. Each filter is observed for 4 orbits each. We here use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB970828 WFPC2 IMAGE WF3 F814W 1 2200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 10] Visit: 10 Visit Priority: Visit Requirements: SEQ 10, 11, 12, 13 WITHIN 5 D SCHED 100% On Hold Comments: Additional Comments: Visits 10, 11, 12 and 13 together form the study of a GRB host in the 814 and 606 filter. Each filter is observed for 12 and 4 orbits each. We here use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000131 WFPC2 IMAGE WF3 F814W 1 2200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 11] Visit: 11 Visit Priority: Visit Requirements: SCHED 100% On Hold Comments: Additional Comments: Visits 10, 11 and 12 together form the study of a GRB host in the 814 filter. Each filter is observed for 4 orbits each. We here use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000131 WFPC2 IMAGE WF3 F814W 1 2200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 12] Visit: 12 Visit Priority: Visit Requirements: SCHED 100% On Hold Comments: Additional Comments: Visits 10, 11 and 12 together form the study of a GRB host in the 814 filter. Each filter is observed for 4 orbits each. We here use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000131 WFPC2 IMAGE WF3 F814W 1 2200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 13] Visit: 13 Visit Priority: Visit Requirements: SCHED 100% On Hold Comments: Additional Comments: Visits 10, 11 and 12 together form the study of a GRB host in the 814 filter. Each filter is observed for 4 orbits each. We here use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000131 WFPC2 IMAGE WF3 F606W 1 2200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 14] Visit: A1 Visit Priority: Visit Requirements: ON HOLD SEQ A1, A2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A1 and A2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010921 WFPC2 IMAGE WFALL F450W 1 800 S PATTERN 10 10 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB010921 WFPC2 IMAGE WFALL F555W 1 800 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB010921 WFPC2 IMAGE WFALL F702W 1 800 S PATTERN 10 30 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 15] Visit: A2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A1 and A2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010921 WFPC2 IMAGE WFALL F814W 1 800 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB010921 WFPC2 IMAGE WFALL F850LP 1 800 S PATTERN 10 50 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 16] Visit: A3 Visit Priority: Visit Requirements: ON HOLD SEQ A3, A4 WITHIN 2 D AFTER A1 BY 8 D TO 12 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A3 and A4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010921 WFPC2 IMAGE WFALL F450W 1 800 S PATTERN 10 10 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB010921 WFPC2 IMAGE WFALL F555W 1 800 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB010921 WFPC2 IMAGE WFALL F702W 1 800 S PATTERN 10 30 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 17] Visit: A4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A3 and A4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010921 WFPC2 IMAGE WFALL F814W 1 800 S PATTERN 10 40 Comments: Dithering by +2.5 in x and +2.5 pixels in y for resolution. Goal is to use these images to determine offset of OT from host center. ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB010921 WFPC2 IMAGE WFALL F850LP 1 800 S PATTERN 10 50 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 18] Visit: A5 Visit Priority: Visit Requirements: ON HOLD SEQ A5, A6 WITHIN 2 D AFTER A1 BY 26 D TO 34 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A5 and A6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010921 WFPC2 IMAGE WFALL F450W 1 800 S PATTERN 10 10 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB010921 WFPC2 IMAGE WFALL F555W 1 800 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB010921 WFPC2 IMAGE WFALL F702W 1 800 S PATTERN 10 30 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 19] Visit: A6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A5 and A6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010921 WFPC2 IMAGE WFALL F814W 1 800 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB010921 WFPC2 IMAGE WFALL F850LP 1 800 S PATTERN 10 50 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 20] Visit: A7 Visit Priority: Visit Requirements: ON HOLD SEQ A7, A8 WITHIN 2 D AFTER A1 BY 55 D TO 65 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A7 and A8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010921 WFPC2 IMAGE WFALL F450W 1 2200 S PATTERN 10 10 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB010921 WFPC2 IMAGE WFALL F555W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 21] Visit: A8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits A7 and A8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB010921 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 30 ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010921 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB010921 WFPC2 IMAGE WFALL F850LP 1 2200 S PATTERN 10 50 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 22] Visit: C0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-3-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% .5Z0.9 UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB-TOO-3-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB-TOO-3-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB-TOO-3-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB-TOO-3-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB-TOO-3-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 23] Visit: C1 Visit Priority: Visit Requirements: ON HOLD SEQ C1, C2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C1 and C2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-3-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-3-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 24] Visit: C2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C1 and C2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-3-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 25] Visit: C3 Visit Priority: Visit Requirements: ON HOLD SEQ C3, C4 WITHIN 2 D AFTER C1 BY 6 D TO 10 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C3 and C4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-3-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-3-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 26] Visit: C4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C3 and C4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-3-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 27] Visit: C5 Visit Priority: Visit Requirements: ON HOLD SEQ C5, C6 WITHIN 2 D AFTER C1 BY 14 D TO 18 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C5 and C6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-3-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-3-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 28] Visit: C6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C5 and C6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-3-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 29] Visit: C7 Visit Priority: Visit Requirements: ON HOLD SEQ C7, C8 WITHIN 2 D AFTER C1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C7 and C8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-3-0 WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 30] Visit: C8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C7 and C8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-3-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 31] Visit: C9 Visit Priority: Visit Requirements: ON HOLD SEQ C9, D0 WITHIN 2 D AFTER C1 BY 123 D TO 133 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C9 and D0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-3-0 WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 32] Visit: D0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits C9 and D0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-3-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 33] Visit: E0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000926 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB000926 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB000926 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB000926 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB000926 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB000926 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 34] Visit: E1 Visit Priority: Visit Requirements: ON HOLD SEQ E1, E2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E1 and E2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000926 WFPC2 IMAGE WFALL F450W 1 2200 S ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB000926 WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 35] Visit: E2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E1 and E2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB000926 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 36] Visit: E3 Visit Priority: Visit Requirements: ON HOLD SEQ E3, E4 WITHIN 2 D AFTER E1 BY 6 D TO 10 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E3 and E4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000926 WFPC2 IMAGE WFALL F450W 1 2200 S ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB000926 WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 37] Visit: E4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E3 and E4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB000926 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 38] Visit: E5 Visit Priority: Visit Requirements: ON HOLD SEQ E5, E6 WITHIN 2 D AFTER E1 BY 14 D TO 18 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E5 and E6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000926 WFPC2 IMAGE WFALL F450W 1 2200 S ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB000926 WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 39] Visit: E6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E5 and E6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB000926 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 40] Visit: E7 Visit Priority: Visit Requirements: ON HOLD SEQ E7, E8 WITHIN 2 D AFTER E1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E7 and E8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000926 WFPC2 IMAGE WFALL F606W CR-SPLIT=NO 3 1000 S PATTERN 10 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 41] Visit: E8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E7 and E8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB000926 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 42] Visit: E9 Visit Priority: Visit Requirements: ON HOLD SEQ E9, F0 WITHIN 2 D AFTER E1 BY 190 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E9 and F0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000926 WFPC2 IMAGE WFALL F450W 1 2200 S ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB000926 WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 43] Visit: F0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits E9 and F0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB000926 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 44] Visit: G0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-Z STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% 0.5 UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB-TOO-4-Z STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG 0.5 UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB-TOO-4-Z STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG 0.5 UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB-TOO-4-Z STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG 0.5 UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB-TOO-4-Z STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG 0.5 UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB-TOO-4-Z STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG 0.5 UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 45] Visit: G1 Visit Priority: Visit Requirements: ON HOLD SEQ G1, G2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G1 and G2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-Z WFPC2 IMAGE WFALL F450W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-4-Z WFPC2 IMAGE WFALL F555W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB-TOO-4-Z WFPC2 IMAGE WFALL F702W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 46] Visit: G2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G1 and G2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-Z WFPC2 IMAGE WFALL F814W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB-TOO-4-Z WFPC2 IMAGE WFALL F850LP 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 47] Visit: G3 Visit Priority: Visit Requirements: ON HOLD SEQ G3, G4 WITHIN 2 D AFTER G1 BY 6 D TO 10 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G3 and G4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-Z WFPC2 IMAGE WFALL F450W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-4-Z WFPC2 IMAGE WFALL F555W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB-TOO-4-Z WFPC2 IMAGE WFALL F702W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 48] Visit: G4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G3 and G4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-Z WFPC2 IMAGE WFALL F814W 1 800 S PATTERN 10 40 0.5 Comments: Dithering by +2.5 in x and +2.5 pixels in y for resolution. Goal is to use these images to determine offset of OT from host center. ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB-TOO-4-Z WFPC2 IMAGE WFALL F850LP 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 49] Visit: G5 Visit Priority: Visit Requirements: ON HOLD SEQ G5, G6 WITHIN 2 D AFTER G1 BY 14 D TO 18 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G5 and G6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-Z WFPC2 IMAGE WFALL F450W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-4-Z WFPC2 IMAGE WFALL F555W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB-TOO-4-Z WFPC2 IMAGE WFALL F702W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 50] Visit: G6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G5 and G6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-Z WFPC2 IMAGE WFALL F814W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB-TOO-4-Z WFPC2 IMAGE WFALL F850LP 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 51] Visit: G7 Visit Priority: Visit Requirements: ON HOLD SEQ G7, G8 WITHIN 2 D AFTER G1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G7 and G8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-Z WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 52] Visit: G8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G7 and G8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-Z WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 53] Visit: G9 Visit Priority: Visit Requirements: ON HOLD SEQ G9, H0 WITHIN 2 D AFTER G1 BY 123 D TO 133 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G9 and H0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-Z WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 54] Visit: H0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits G9 and H0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-Z WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 55] Visit: I0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% .5Z0.9 UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB-TOO-4-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB-TOO-4-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB-TOO-4-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB-TOO-4-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB-TOO-4-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 56] Visit: I1 Visit Priority: Visit Requirements: ON HOLD SEQ I1, I2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I1 and I2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-4-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 57] Visit: I2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I1 and I2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 58] Visit: I3 Visit Priority: Visit Requirements: ON HOLD SEQ I3, I4 WITHIN 2 D AFTER I1 BY 6 D TO 10 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I3 and I4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-4-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 59] Visit: I4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I3 and I4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 60] Visit: I5 Visit Priority: Visit Requirements: ON HOLD SEQ I5, I6 WITHIN 2 D AFTER I1 BY 14 D TO 18 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I5 and I6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-4-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 61] Visit: I6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I5 and I6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 62] Visit: I7 Visit Priority: Visit Requirements: ON HOLD SEQ I7, I8 WITHIN 2 D AFTER I1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I7 and I8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-0 WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 63] Visit: I8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I7 and I8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 64] Visit: I9 Visit Priority: Visit Requirements: ON HOLD SEQ I9, J0 WITHIN 2 D AFTER I1 BY 123 D TO 133 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I9 and J0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-4-0 WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 65] Visit: J0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits I9 and J0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-4-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 66] Visit: K0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010222 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB010222 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB010222 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB010222 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB010222 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB010222 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 67] Visit: K1 Visit Priority: Visit Requirements: ON HOLD SEQ K1, K2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K1 and K2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010222 WFPC2 IMAGE WFALL F450W 1 2200 S ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB010222 WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 68] Visit: K2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K1 and K2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010222 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 69] Visit: K3 Visit Priority: Visit Requirements: ON HOLD SEQ K3, K4 WITHIN 2 D AFTER K1 BY 13 D TO 21 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K3 and K4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010222 WFPC2 IMAGE WFALL F450W 1 2200 S ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB010222 WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 70] Visit: K4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K3 and K4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010222 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 71] Visit: K5 Visit Priority: Visit Requirements: ON HOLD SEQ K5, K6 WITHIN 2 D AFTER K1 BY 35 D TO 46 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K5 and K6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010222 WFPC2 IMAGE WFALL F450W 1 2200 S ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB010222 WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 72] Visit: K6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K5 and K6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010222 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 73] Visit: K7 Visit Priority: Visit Requirements: ON HOLD SEQ K7, K8 WITHIN 2 D AFTER K1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K7 and K8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010222 WFPC2 IMAGE WFALL F606W CR-SPLIT=NO 3 1000 S PATTERN 10 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 74] Visit: K8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K7 and K8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010222 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 75] Visit: K9 Visit Priority: Visit Requirements: ON HOLD SEQ K9, L0, L1 WITHIN 2 D AFTER K1 BY 190 D TO 210 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K9, L0 and L1 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB010222 WFPC2 IMAGE WFALL F450W CR-SPLIT=NO 3 1000 S PATTERN 10 10 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 76] Visit: L0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K9 and L0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB010222 WFPC2 IMAGE WFALL F606W CR-SPLIT=NO 3 1000 S PATTERN 10 40 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 77] Visit: L1 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits K9 and L0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 70 GRB010222 WFPC2 IMAGE WFALL F814W CR-SPLIT=NO 3 1000 S PATTERN 10 70 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 78] Visit: M0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-Z STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% 0.5 UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB-TOO-5-Z STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG 0.5 UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB-TOO-5-Z STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG 0.5 UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB-TOO-5-Z STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG 0.5 UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB-TOO-5-Z STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG 0.5 UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB-TOO-5-Z STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG 0.5 UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 79] Visit: M1 Visit Priority: Visit Requirements: ON HOLD SEQ M1, M2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M1 and M2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-Z WFPC2 IMAGE WFALL F450W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-Z WFPC2 IMAGE WFALL F555W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB-TOO-5-Z WFPC2 IMAGE WFALL F702W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 80] Visit: M2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M1 and M2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-Z WFPC2 IMAGE WFALL F814W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB-TOO-5-Z WFPC2 IMAGE WFALL F850LP 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 81] Visit: M3 Visit Priority: Visit Requirements: ON HOLD SEQ M3, M4 WITHIN 2 D AFTER M1 BY 6 D TO 10 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M3 and M4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-Z WFPC2 IMAGE WFALL F450W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-Z WFPC2 IMAGE WFALL F555W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB-TOO-5-Z WFPC2 IMAGE WFALL F702W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 82] Visit: M4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M3 and M4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-Z WFPC2 IMAGE WFALL F814W 1 800 S PATTERN 10 40 0.5 Comments: Dithering by +2.5 in x and +2.5 pixels in y for resolution. Goal is to use these images to determine offset of OT from host center. ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB-TOO-5-Z WFPC2 IMAGE WFALL F850LP 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 83] Visit: M5 Visit Priority: Visit Requirements: ON HOLD SEQ M5, M6 WITHIN 2 D AFTER M1 BY 14 D TO 18 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M5 and M6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-Z WFPC2 IMAGE WFALL F450W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-Z WFPC2 IMAGE WFALL F555W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 30 GRB-TOO-5-Z WFPC2 IMAGE WFALL F702W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 84] Visit: M6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M5 and M6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-Z WFPC2 IMAGE WFALL F814W 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 50 GRB-TOO-5-Z WFPC2 IMAGE WFALL F850LP 1 2200 S 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 85] Visit: M7 Visit Priority: Visit Requirements: ON HOLD SEQ M7, M8 WITHIN 2 D AFTER M1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M7 and M8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-Z WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 86] Visit: M8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M7 and M8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-Z WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 87] Visit: M9 Visit Priority: Visit Requirements: ON HOLD SEQ M9, N0 WITHIN 2 D AFTER M1 BY 123 D TO 133 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M9 and N0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-Z WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 88] Visit: N0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits M9 and N0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-Z WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 0.5 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 89] Visit: O0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% .5Z0.9 UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB-TOO-5-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB-TOO-5-0 STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB-TOO-5-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB-TOO-5-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB-TOO-5-0 STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG .5Z0.9 UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 90] Visit: O1 Visit Priority: Visit Requirements: ON HOLD SEQ O1, O2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O1 and O2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 91] Visit: O2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O1 and O2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 92] Visit: O3 Visit Priority: Visit Requirements: ON HOLD SEQ O3, O4 WITHIN 2 D AFTER O1 BY 6 D TO 10 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O3 and O4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 93] Visit: O4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O3 and O4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 94] Visit: O5 Visit Priority: Visit Requirements: ON HOLD SEQ O5, O6 WITHIN 2 D AFTER O1 BY 14 D TO 18 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O5 and O6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-0 WFPC2 IMAGE WFALL F555W 1 2200 S .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-0 WFPC2 IMAGE WFALL F702W 1 2200 S PATTERN 10 20 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 95] Visit: O6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O5 and O6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 96] Visit: O7 Visit Priority: Visit Requirements: ON HOLD SEQ O7, O8 WITHIN 2 D AFTER O1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O7 and O8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-0 WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 97] Visit: O8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O7 and O8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 98] Visit: O9 Visit Priority: Visit Requirements: ON HOLD SEQ O9, P0 WITHIN 2 D AFTER O1 BY 123 D TO 133 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O9 and P0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-0 WFPC2 IMAGE WFALL F702W CR-SPLIT=NO 3 1000 S PATTERN 10 10 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [ 99] Visit: P0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits O9 and P0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-0 WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 .5Z0.9 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [100] Visit: Q0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: STIS UV imaging of the optical transient to (combined with ground-based optical/IR and X-ray measurements) determine the effect of dust within the host (determination of the curvature of the spectrum due to reddening). These observations have to be scheduled roughly ~ 1 week from the GRB event. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-D STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% UST UV-MAM A ------------------------------------------------------------------------------------------------------------------------------------ 11 GRB-TOO-5-D STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG UST UV-MAM 0.246, 0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 12 GRB-TOO-5-D STIS/N ACCUM F25QTZ MIRROR 1 800 S MAX DUR 120% POS TARG UST UV-MAM 0.369, 0.369 A ------------------------------------------------------------------------------------------------------------------------------------ 13 GRB-TOO-5-D STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UST UV-MAM 0.123, 0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 14 GRB-TOO-5-D STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UST UV-MAM -0.246,-0.123 A ------------------------------------------------------------------------------------------------------------------------------------ 15 GRB-TOO-5-D STIS/N ACCUM F25QTZ MIRROR 1 866 S MAX DUR 120% POS TARG UST UV-MAM -0.123,-0.246 A ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [101] Visit: Q1 Visit Priority: Visit Requirements: ON HOLD SEQ Q1, Q2 WITHIN 2 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q1 and Q2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-D WFPC2 IMAGE WFALL F450W 1 2200 S UST ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-D WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [102] Visit: Q2 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q1 and Q2 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-D WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [103] Visit: Q3 Visit Priority: Visit Requirements: ON HOLD SEQ Q3, Q4 WITHIN 2 D AFTER Q1 BY 6 D TO 10 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q3 and Q4 together form the 2nd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-D WFPC2 IMAGE WFALL F450W 1 2200 S UST ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-D WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [104] Visit: Q4 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q3 and Q4 together form the first epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-D WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [105] Visit: Q5 Visit Priority: Visit Requirements: ON HOLD SEQ Q5, Q6 WITHIN 2 D AFTER Q1 BY 14 D TO 18 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q5 and Q6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-D WFPC2 IMAGE WFALL F450W 1 2200 S UST ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB-TOO-5-D WFPC2 IMAGE WFALL F606W 1 2200 S PATTERN 10 20 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [106] Visit: Q6 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q5 and Q6 together form the 3rd epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-D WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [107] Visit: Q7 Visit Priority: Visit Requirements: ON HOLD SEQ Q7, Q8 WITHIN 2 D AFTER Q1 BY 63 D TO 73 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q7 and Q8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-D WFPC2 IMAGE WFALL F606W CR-SPLIT=NO 3 1000 S PATTERN 10 10 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [108] Visit: Q8 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q7 and Q8 together form the 4th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-D WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [109] Visit: Q9 Visit Priority: Visit Requirements: ON HOLD SEQ Q9, R0 WITHIN 2 D AFTER Q1 BY 123 D TO 133 D SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q9 and R0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB-TOO-5-D WFPC2 IMAGE WFALL F606W CR-SPLIT=NO 3 1000 S PATTERN 10 10 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [110] Visit: R0 Visit Priority: Visit Requirements: ON HOLD SCHED 100% On Hold Comments: Target of Opportunity Additional Comments: Visits Q9 and R0 together form the 5th epoch of a series of 5 epochs at roughly tp-8, tp, tp+8, tp+60 and tp+120 days, where tp is the expected epoch of maximum light of the supernova that possibly acompanies the gamma- ray burst. The observations are made using two broad band filters. In case we find from earlier observations that the source is very faint, we will contact STScI and request that the observations be made in a single filter. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 40 GRB-TOO-5-D WFPC2 IMAGE WFALL F814W 1 2200 S PATTERN 10 40 UST ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [111] Visit: S0 Visit Priority: Visit Requirements: On Hold Comments: Additional Comments: Visits S0 is the study of a GRB host in the 606 and 814 filters. Each filter is observed for 2 orbits each. We h ere use the BOX pattern that offsets in steps of 2.5 WF pixels. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 GRB000630 WFPC2 IMAGE WF3 F606W CR-SPLIT=NO 1 1200 S PATTERN 20 10 ------------------------------------------------------------------------------------------------------------------------------------ 20 GRB000630 WFPC2 IMAGE WF3 F814W CR-SPLIT=NO 1 1200 S PATTERN 20 20 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [112] Visit: T1 Visit Priority: Visit Requirements: On Hold Comments: Additional Comments: Visit T1 is the first in a series of STIS visits on GRB011211 Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 615 S PATTERN 60 1 CD ------------------------------------------------------------------------------------------------------------------------------------ 2 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 60 S CD ------------------------------------------------------------------------------------------------------------------------------------ 3 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 668 S PATTERN 60 3 POS TARG CD 1.0142, 1.0142 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [113] Visit: T2 Visit Priority: Visit Requirements: SCHED 100% AFTER T1 BY 7 D TO 14 D On Hold Comments: Additional Comments: Visit T2 is the second in a series of STIS visits on GRB0112 11 Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 564 S PATTERN 60 1 CD ------------------------------------------------------------------------------------------------------------------------------------ 2 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 60 S CD ------------------------------------------------------------------------------------------------------------------------------------ 3 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 617 S PATTERN 60 3 POS TARG CD 1.0142, 1.0142 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [114] Visit: T3 Visit Priority: Visit Requirements: SCHED 100% AFTER T1 BY 14 D TO 21 D On Hold Comments: Additional Comments: Visit T3 is the second in a series of STIS visits on GRB0112 11 Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 564 S PATTERN 60 1 CD ------------------------------------------------------------------------------------------------------------------------------------ 2 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 60 S CD ------------------------------------------------------------------------------------------------------------------------------------ 3 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 617 S PATTERN 60 3 POS TARG CD 1.0142, 1.0142 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [115] Visit: T4 Visit Priority: Visit Requirements: SCHED 100% AFTER T1 BY 44 D TO 51 D On Hold Comments: Additional Comments: Visit T4 is the last in a series of STIS visits on GRB011211. Here, we observe for 3 orbits to get a better detection of the host galaxy. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 564 S PATTERN 60 1 CD ------------------------------------------------------------------------------------------------------------------------------------ 2 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 60 S CD ------------------------------------------------------------------------------------------------------------------------------------ 3 GRB011211 STIS/C ACCUM 50CCD MIRROR GAIN=1,CR-SPLIT=NO 1 616 S PATTERN 60 3 POS TARG CD 1.0142, 1.0142 ------------------------------------------------------------------------------------------------------------------------------------ 8867( 21) - 12/14/01 17:23 - [116] Summary Form for Proposal 8867 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures WF3 WFALL F25QTZ 50CCD ------------------------------------------------------------------------------------------------------------------------------------ Configurations WFPC2 STIS/NUV-MAMA STIS/CCD ------------------------------------------------------------------------------------------------------------------------------------ Opmodes IMAGE ACCUM ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters CR-SPLIT=NO GAIN=1 ------------------------------------------------------------------------------------------------------------------------------------ Proposal Category GO ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements SEQ 01, 02, 03 WITHIN 3 D SCHED 100% PATTERN 20 10 SCHED 100% SEQ 10, 11, 12, 13 WITHIN 5 D SCHED 100% ON HOLD SEQ A1, A2 WITHIN 2 D SCHED 100% PATTERN 10 10 PATTERN 10 20 PATTERN 10 30 ON HOLD SCHED 100% PATTERN 10 40 PATTERN 10 50 ON HOLD SEQ A3, A4 WITHIN 2 D AFTER A1 BY 8 D TO 12 D SCHED 100% ON HOLD SEQ A5, A6 WITHIN 2 D AFTER A1 BY 26 D TO 34 D SCHED 100% ON HOLD SEQ A7, A8 WITHIN 2 D AFTER A1 BY 55 D TO 65 D SCHED 100% MAX DUR 120% MAX DUR 120% POS TARG 0.246, 0.123 MAX DUR 120% POS TARG 0.369, 0.369 MAX DUR 120% POS TARG 0.123, 0.246 MAX DUR 120% POS TARG -0.246,-0.123 MAX DUR 120% POS TARG -0.123,-0.246 ON HOLD SEQ C1, C2 WITHIN 2 D SCHED 100% ON HOLD SEQ C3, C4 WITHIN 2 D AFTER C1 BY 6 D TO 10 D SCHED 100% ON HOLD SEQ C5, C6 WITHIN 2 D AFTER C1 BY 14 D TO 18 D SCHED 100% ON HOLD SEQ C7, C8 WITHIN 2 D AFTER C1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ C9, D0 WITHIN 2 D AFTER C1 BY 123 D TO 133 D SCHED 100% ON HOLD SEQ E1, E2 WITHIN 2 D SCHED 100% ON HOLD SEQ E3, E4 WITHIN 2 D AFTER E1 BY 6 D TO 10 D SCHED 100% ON HOLD SEQ E5, E6 WITHIN 2 D AFTER E1 BY 14 D TO 18 D SCHED 100% ON HOLD SEQ E7, E8 WITHIN 2 D AFTER E1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ E9, F0 WITHIN 2 D AFTER E1 BY 190 D SCHED 100% ON HOLD SEQ G1, G2 WITHIN 2 D SCHED 100% ON HOLD SEQ G3, G4 WITHIN 2 D AFTER G1 BY 6 D TO 10 D SCHED 100% ON HOLD SEQ G5, G6 WITHIN 2 D AFTER G1 BY 14 D TO 18 D SCHED 100% ON HOLD SEQ G7, G8 WITHIN 2 D AFTER G1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ G9, H0 WITHIN 2 D AFTER G1 BY 123 D TO 133 D SCHED 100% ON HOLD SEQ I1, I2 WITHIN 2 D SCHED 100% ON HOLD SEQ I3, I4 WITHIN 2 D AFTER I1 BY 6 D TO 10 D SCHED 100% ON HOLD SEQ I5, I6 WITHIN 2 D AFTER I1 BY 14 D TO 18 D SCHED 100% ON HOLD SEQ I7, I8 WITHIN 2 D AFTER I1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ I9, J0 WITHIN 2 D AFTER I1 BY 123 D TO 133 D SCHED 100% ON HOLD SEQ K1, K2 WITHIN 2 D SCHED 100% ON HOLD SEQ K3, K4 WITHIN 2 D AFTER K1 BY 13 D TO 21 D SCHED 100% ON HOLD SEQ K5, K6 WITHIN 2 D AFTER K1 BY 35 D TO 46 D SCHED 100% ON HOLD SEQ K7, K8 WITHIN 2 D AFTER K1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ K9, L0, L1 WITHIN 2 D AFTER K1 BY 190 D TO 210 D SCHED 100% PATTERN 10 70 ON HOLD SEQ M1, M2 WITHIN 2 D SCHED 100% ON HOLD SEQ M3, M4 WITHIN 2 D AFTER M1 BY 6 D TO 10 D SCHED 100% ON HOLD SEQ M5, M6 WITHIN 2 D AFTER M1 BY 14 D TO 18 D SCHED 100% ON HOLD SEQ M7, M8 WITHIN 2 D AFTER M1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ M9, N0 WITHIN 2 D AFTER M1 BY 123 D TO 133 D SCHED 100% ON HOLD SEQ O1, O2 WITHIN 2 D SCHED 100% ON HOLD SEQ O3, O4 WITHIN 2 D AFTER O1 BY 6 D TO 10 D SCHED 100% ON HOLD SEQ O5, O6 WITHIN 2 D AFTER O1 BY 14 D TO 18 D SCHED 100% ON HOLD SEQ O7, O8 WITHIN 2 D AFTER O1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ O9, P0 WITHIN 2 D AFTER O1 BY 123 D TO 133 D SCHED 100% ON HOLD SEQ Q1, Q2 WITHIN 2 D SCHED 100% ON HOLD SEQ Q3, Q4 WITHIN 2 D AFTER Q1 BY 6 D TO 10 D SCHED 100% ON HOLD SEQ Q5, Q6 WITHIN 2 D AFTER Q1 BY 14 D TO 18 D SCHED 100% ON HOLD SEQ Q7, Q8 WITHIN 2 D AFTER Q1 BY 63 D TO 73 D SCHED 100% ON HOLD SEQ Q9, R0 WITHIN 2 D AFTER Q1 BY 123 D TO 133 D SCHED 100% PATTERN 20 20 PATTERN 60 1 PATTERN 60 3 POS TARG 1.0142, 1.0142 SCHED 100% AFTER T1 BY 7 D TO 14 D SCHED 100% AFTER T1 BY 14 D TO 21 D SCHED 100% AFTER T1 BY 44 D TO 51 D ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements F450W F606W F814W F555W F702W F850LP MIRROR ------------------------------------------------------------------------------------------------------------------------------------ Target Names GRB970828 GRB000131 GRB010921 GRB-TOO-3-0.5Z0.9 GRB000926 GRB-TOO-4-Z0.5 GRB-TOO-4-0.5Z0.9 GRB010222 GRB-TOO-5-Z0.5 GRB-TOO-5-0.5Z0.9 GRB-TOO-5-DUST GRB000630 GRB011211 ------------------------------------------------------------------------------------------------------------------------------------