15673( 2) - 08-Jan-2019 13:11:41 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 15673 Version: 2 Check-in Time: 08-Jan-2019 13:11:41 STScI Edit Number: 0 Title Shining light on obscuring outflows in AGN ------------------------------------------------------------------------------------ Type Cycle GO 26 ------------------------------------------------------------------------------------ Investigators Contact? PI: Dr. Jelle Kaastra Space Research Organization Netherlands Y CoI: Dr. Gerard A. Kriss Space Telescope Science Institute N CoI: Dr. Massimo Cappi INAF, Istituto di Fisica Spaziale e Fisica N Cosmica-Bologna CoI: Dr. Nahum Arav Virginia Polytechnic Institute and State N University CoI: Dr. Ehud Behar Technion-Israel Institute of Technology N CoI: Prof. Stefano Bianchi Universita' degli Studi Roma Tre N CoI: Dr. Graziella Branduardi-Raymont University College London N CoI: Dr. Elisa Costantini Space Research Organization Netherlands N CoI: Dr. Laura di Gesu INTEGRAL Science Data Centre (ISDC) N CoI: Dr. Barbara De Marco Nicolaus Copernicus Astronomical Center N CoI: Dr. Jacobo Ebrero ESA-European Space Astronomy Centre N CoI: Dr. Shai Kaspi Tel Aviv University - Wise Observatory N CoI: Mr. Junjie Mao Space Research Organization Netherlands N CoI: Prof. Giorgio Matt Universita' degli Studi Roma Tre N CoI: Dr. Missagh Mehdipour Space Research Organization Netherlands N CoI: Dr. Stephane Paltani Observatoire de Geneve N CoI: Dr. Pierre-Olivier Petrucci Institut de Planetologie et N d'Astrophysique de Grenoble CoI: Dr. Ciro Pinto University of Cambridge N CoI: Dr. Gabriele Ponti Max-Planck-Institut fur extraterrestrische N Physik CoI: Dr. Dominic Walton University of Cambridge N ------------------------------------------------------------------------------------ Abstract AGN can be obscured by gas streams close to the black hole that shield remote regions from ionising radiation. We witnessed such an event in NGC 5548 and NGC 3783 where 90% of the soft X-rays are blocked by a dense gas stream close to the BLR. Our joint observations with XMM-Newton, NuSTAR and HST/COS showed UV broad absorption lines associated with the X-ray absorption and allowed us to characterise this unique obscuration event completely. We propose to investigate a similar event in another Seyfert 1 using the same instruments. Swift monitoring (98 ks) will be used to find the event, which will be characterised by joint ToO observations with XMM-Newton (150 ks), HST/COS (4 orbits) and NuSTAR (50 ks). ------------------------------------------------------------------------------------ Observations Description ------------------------ We will observe a Seyfert 1 galaxy that has entered an obscured phase similar to NGC 5548, NGC 985, or Mrk 335 in order to use simultaneous XMM-Newton, NuSTAR, and HST/COS observations to measure the physical characteristics of the 15673( 2) - 08-Jan-2019 13:11:41 - [ 2] outflow causing the obscuration. Our observations will be triggered via a monitoring program conducted on 7 bright Seyfert 1 galaxies with Swift. The first XMM-Newton observation will be as soon as possible after the trigger and 100 ks in duration in order to have well-determined obscurer parameters. An additional observation of 50 ks following the first observation but before the end of the XMM visibility window will enable us to study the variability of the obscurer. As nearly simultaneous with each XMM visit as possible, we will observe for 25 ks with NuSTAR and for 2 orbits with HST/COS. Our COS observations will use gratings G130M and G160M in order to observe the main absorption line transitions in C III* 1176, Ly alpha, N V, Si IV, and C IV. Our previous observational campaigns on Mrk 279, Mrk 509, NGC 5548, and NGC 985 all achieved good results with a signal-to-noise ratio of 20 per resolution element in the continuum for these objects. To achieve a 4-fold diversity of grating settings for each grating, we use all 4 FP-POS positions with CENWAVE=1222 for G130M. For G160M, we use CENWAVES 1533 and 1629 to cover the full FUV wavelength range and to span the gap between segments A and B. We use 2 FP-POS positions for each CENWAVE. To outline the ETC calculations for our potential targets, we tabulate results for all 8 here. (Fluxes are obtained from Dunn et al. 2006, PASP, 118, 572, and from the MAST archive.) Source z E(B-V) Min_Flam Max_Flam Mean_Flam NGC 3227 0.003859 0.020 0.05e-14 0.4e-14 0.12e-14 NGC 4593 0.00900 0.022 0.5e-14 2.4e-14 1.5e-14 Mrk 841 0.036422 0.026 2.0e-14 4.3e-14 3.2e-14 Mrk 509 0.034397 0.051 4.1e-14 1.4e-13 9.0e-14 Ark 564 0.024684 0.053 0.6e-14 1.0e-14 0.8e-14 MR2251-178 0.063980 0.035 1.8e-14 4.7e-14 3.3e-14 NGC 7469 0.016317 0.061 2.7e-14 7.1e-14 4.9e-14 We note that our triggered TOO observation will observe only *one* of these objects. These observations pose no bright object concerns. All historical flux levels for each of the AGN in our sample lie below the bright object limits for COS. Since all of these objects have been observed successfully before using either COS or STIS, there are also no surrounding field objects that are too bright. All of our targets are faint enough that we can use an imaging target acquisition with Mirror B, except for Mrk 509, for which we use a spectroscopic target acquisition. Rather than do a separate ETC check on bright object constraints for each AGN, we simply show here calculations for the brightest object for which we do an imaging target acquisition, NGC 7469, and the brightest overall, Mrk 509. (We note that the only AGN that could ever violate the COS brightness limits are NGC 4151 and 3C 273.) Our ETC calculations use the ETC FOS quasar spectrum redshifted appropriately with foreground Milky Way extinction from NED. Here we show calculations relevant for the minimum and maximum fluxes expected (Dunn et al. 2006) in order to get our limiting cases: 15673( 2) - 08-Jan-2019 13:11:41 - [ 3] - ACQUISITION (for Mrk 509)- Configuration Flux EXP time Max cts/s/pix Total rate Buffer Time COS ETC ID G130M/1291 0.5e-14 11.0 s 0.10 504 4679 COS.sa.1306938 G130M/1291 1.4e-13 0.4 s 0.13 5570 423 COS.sa.1306936 - ACQUISITION (for MR2251-178)- Configuration Flux EXP time Max cts/s/pix Total rate COS ETC ID PSA/Mirror B 1.8e-14 6.6 s 8 1011 COS.ta.1306935 PSA/Mirror B 4.7e-14 2.5 s 22 1156 COS.ta.1306930 - ACQUISITION (for NGC 3227)- Configuration Flux EXP time Max cts/s/pix Total rate COS ETC ID PSA/Mirror B 0.05e-14 131 s 0.4 925 COS.ta.1306969 PSA/Mirror B 0.4e-14 16.0 s 4 958 COS.ta.1306973 - EXPOSURES (for Mrk 509)- Configuration Flux EXP time Max cts/s/pix Total rate Buffer Time COS ETC ID G130M/1222 5.0e-14 1000 0.01 236 10011 COS.sp.1306947 G130M/1222 1.4e-13 1000 0.03 4663 505 COS.sp.1306941 G160M/1533 5.0e-14 1000 0.001 168 14027 COS.sp.1306951 G160M/1533 1.4e-13 1000 0.032 3232 729 COS.sp.1306954 Although it is recommended to use a BUFFER-TIME that is 2/3 of that given by the ETC, our general strategy is to choose a value that is less than that, and also an integer divisor of the exposure time minus 110 s. This minimizes the overhead between exposures while doing buffer dumps, e.g., BUFFER-TIME = (Exposure Time - 110) / n ------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 4] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-3227 GALAXY, ACCRETION DISK, RA=10H23M30.5700S +/- 0.1", J2000 Z = V = 11.75 +/- 0.5 F(1368)=0.3e-14 BLR, NLR, SEYFERT, WIND DEC=+19D51'54.30" +/- 0.1" 0.003859 Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-4593 GALAXY, ACCRETION DISK, RA=12H39M39.4920S +/- 0.1", J2000 Z = V = 13.15 +/- 0.5 F(1368)=1.5e-14 BLR, NLR, SEYFERT, WIND DEC=-05D20'39.16" +/- 0.1" 0.00900 Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------------------------------------------------------------ 3 MRK-841 GALAXY, ACCRETION DISK, RA=15H04M1.1720S +/- 0.1", J2000 Z = V = 14.27 +/- 0.5 F(1368)=3.2e-14 BLR, NLR, SEYFERT, WIND DEC=+10D26'16.45" +/- 0.1" 0.036422 Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------------------------------------------------------------ 4 MRK-509 GALAXY, ACCRETION DISK, RA=20H44M9.7681S +/- 0.1", J2000 Z = V = 13.12 +/- 0.5 F(1368)=9.0e-14 BLR, NLR, SEYFERT, WIND DEC=-10D43'24.44" +/- 0.1" 0.034397 Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------------------------------------------------------------ 5 ARK-564 GALAXY, ACCRETION DISK, RA=22H42M39.3090S +/- 0.1", J2000 Z = V = 14.16 +/- 0.5 F(1368)=0.8e-14 BLR, NLR, SEYFERT, WIND DEC=+29D43'31.55" +/- 0.1" 0.024684 Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------------------------------------------------------------ 6 MR-2251-178 GALAXY, ACCRETION DISK, RA=22H54M5.8959S +/- 0.1", J2000 Z = V = 14.36 +/- 0.5 F(1368)=3.3e-14 BLR, NLR, SEYFERT, WIND DEC=-17D34'55.10" +/- 0.1" 0.063980 Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------------------------------------------------------------ 7 NGC-7469 GALAXY, ACCRETION DISK, RA=23H03M15.6740S +/- 0.1", J2000 Z = V = 12.34 +/- 0.5 F(1368)=4.9e-14 BLR, NLR, SEYFERT, WIND DEC=+08D52'25.28" +/- 0.1" 0.016317 Reference Frame: ICRS Extended: NO Comments: This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 5] Visit: 01 (1A) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-3227 COS/NUV ACQ/IMA PSA MIRRORB 1 131 S (131 GE S) Comments: Exposure time is chosen for the faintest historical flux, 0.05e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-3227 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=3000, FP-POS=ALL 1 415 S G (1660 S) ------------------------------------------------------------------------------------------------------------------------------------ 3 NGC-3227 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) ------------------------------------------------------------------------------------------------------------------------------------ 4 NGC-3227 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) ------------------------------------------------------------------------------------------------------------------------------------ 5 NGC-3227 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) ------------------------------------------------------------------------------------------------------------------------------------ 6 NGC-3227 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-3227 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G NGC-3227 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-3227 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 6] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-3227 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G NGC-3227 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 7] Visit: 02 (1B) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-3227 COS/NUV ACQ/IMA PSA MIRRORB 1 131 S (131 GE S) Comments: Exposure time is chosen for the faintest historical flux, 0.05e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-3227 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=3000, FP-POS=ALL 1 415 S G (1660 S) ------------------------------------------------------------------------------------------------------------------------------------ 3 NGC-3227 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) ------------------------------------------------------------------------------------------------------------------------------------ 4 NGC-3227 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) ------------------------------------------------------------------------------------------------------------------------------------ 5 NGC-3227 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) ------------------------------------------------------------------------------------------------------------------------------------ 6 NGC-3227 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-3227 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G NGC-3227 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G NGC-3227 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-3227 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 8] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-3227 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G NGC-3227 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 9] Visit: 03 (2A) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-4593 COS/NUV ACQ/IMA PSA MIRRORB 1 14 S (14 GE S) Comments: Exposure time is chosen for the faintest historical flux, 0.5e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-4593 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=355, FP-POS=ALL 1 465 S G (1860 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 3 NGC-4593 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 NGC-4593 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 NGC-4593 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 10] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 NGC-4593 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-4593 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G NGC-4593 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-4593 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-4593 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G NGC-4593 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 11] Visit: 04 (2B) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-4593 COS/NUV ACQ/IMA PSA MIRRORB 1 14 S (14 GE S) Comments: Exposure time is chosen for the faintest historical flux, 0.5e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-4593 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=355, FP-POS=ALL 1 465 S G (1860 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 3 NGC-4593 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 NGC-4593 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 NGC-4593 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 12] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 NGC-4593 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-4593 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G NGC-4593 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G NGC-4593 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-4593 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-4593 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G NGC-4593 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 13] Visit: 05 (3A) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 MRK-841 COS/NUV ACQ/IMA PSA MIRRORB 1 3.3 S (3.3 GE S) Comments: Exposure time is chosen for the faintest historical flux, 2.0e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 MRK-841 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=361, FP-POS=ALL 1 471 S G (1884 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 3 MRK-841 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 MRK-841 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 MRK-841 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 14] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 MRK-841 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ MRK-841 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G MRK-841 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-841 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-841 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G MRK-841 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 15] Visit: 06 (3B) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 MRK-841 COS/NUV ACQ/IMA PSA MIRRORB 1 3.3 S (3.3 GE S) Comments: Exposure time is chosen for the faintest historical flux, 2.0e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 MRK-841 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=361, FP-POS=ALL 1 471 S G (1884 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 3 MRK-841 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 MRK-841 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 MRK-841 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 16] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 MRK-841 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ MRK-841 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G MRK-841 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G MRK-841 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-841 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-841 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G MRK-841 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 17] Visit: 07 (4A) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 MRK-509 COS/FUV ACQ/PEA PSA G130M 1291 1 11 S (11 KXD S) Comments: Exposure time is chosen for the faintest historical flux, 0.5e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 MRK-509 COS/FUV ACQ/PEA PSA G130M 1291 NUM-POS=5, STEP-SIZE=0.9, 1 11 S (11 KD CENTER=FLUX-WT-FLR S) Comments: Exposure time is chosen for the faintest historical flux, 0.5e-14. ------------------------------------------------------------------------------------------------------------------------------------ 3 MRK-509 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=300, FP-POS=ALL 1 410 S G (1640 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 MRK-509 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 MRK-509 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 6 MRK-509 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 15673( 2) - 08-Jan-2019 13:11:41 - [ 18] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ 7 MRK-509 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ MRK-509 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD MRK-509 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G MRK-509 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-509 5 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-509 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G MRK-509 7 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 19] Visit: 08 (4B) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 MRK-509 COS/FUV ACQ/PEA PSA G130M 1291 1 11 S (11 KXD S) Comments: Exposure time is chosen for the faintest historical flux, 0.5e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 MRK-509 COS/FUV ACQ/PEA PSA G130M 1291 NUM-POS=5, STEP-SIZE=0.9, 1 11 S (11 KD CENTER=FLUX-WT-FLR S) Comments: Exposure time is chosen for the faintest historical flux, 0.5e-14. ------------------------------------------------------------------------------------------------------------------------------------ 3 MRK-509 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=300, FP-POS=ALL 1 410 S G (1640 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 MRK-509 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 MRK-509 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 20] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 MRK-509 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 7 MRK-509 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ MRK-509 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD MRK-509 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G MRK-509 3 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G MRK-509 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-509 5 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MRK-509 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G MRK-509 7 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 21] Visit: 09 (5A) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 ARK-564 COS/NUV ACQ/IMA PSA MIRRORB 1 10.7 S GE (10.7 S) Comments: Exposure time is chosen for the faintest historical flux, 0.6e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 ARK-564 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=358, FP-POS=ALL 1 468 S G (1872 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 3 ARK-564 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 ARK-564 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 ARK-564 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 22] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 ARK-564 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ ARK-564 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G ARK-564 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G ARK-564 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G ARK-564 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G ARK-564 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 23] Visit: 10 (5B) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 ARK-564 COS/NUV ACQ/IMA PSA MIRRORB 1 10.7 S GE (10.7 S) Comments: Exposure time is chosen for the faintest historical flux, 0.6e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 ARK-564 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=358, FP-POS=ALL 1 468 S G (1872 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 3 ARK-564 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 ARK-564 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 ARK-564 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 24] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 ARK-564 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ ARK-564 1 COS/NUV ACQ/IMA PSA MIRRORB none none none none 1 N/A GE ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G ARK-564 2 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G ARK-564 3 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G ARK-564 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G ARK-564 5 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G ARK-564 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 25] Visit: 11 (6A) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 MR-2251-178 COS/FUV ACQ/PEA PSA G130M 1291 1 6.6 S (6.6 KXD S) Comments: Exposure time is chosen for the faintest historical flux, 1.8e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 MR-2251-178 COS/FUV ACQ/PEA PSA G130M 1291 NUM-POS=5, STEP-SIZE=0.9, 1 6.6 S (6.6 KD CENTER=FLUX-WT-FLR S) Comments: Exposure time is chosen for the faintest historical flux, 1.8e-14. ------------------------------------------------------------------------------------------------------------------------------------ 3 MR-2251-178 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=309, FP-POS=ALL 1 419 S G (1676 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 MR-2251-178 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 MR-2251-178 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 6 MR-2251-178 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 15673( 2) - 08-Jan-2019 13:11:41 - [ 26] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ 7 MR-2251-178 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ MR-2251-178 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD MR-2251-178 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G MR-2251-178 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MR-2251-178 5 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MR-2251-178 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G MR-2251-178 7 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 27] Visit: 12 (6B) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 MR-2251-178 COS/FUV ACQ/PEA PSA G130M 1291 1 6.6 S (6.6 KXD S) Comments: Exposure time is chosen for the faintest historical flux, 1.8e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 MR-2251-178 COS/FUV ACQ/PEA PSA G130M 1291 NUM-POS=5, STEP-SIZE=0.9, 1 6.6 S (6.6 KD CENTER=FLUX-WT-FLR S) Comments: Exposure time is chosen for the faintest historical flux, 1.8e-14. ------------------------------------------------------------------------------------------------------------------------------------ 3 MR-2251-178 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=309, FP-POS=ALL 1 419 S G (1676 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 MR-2251-178 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 MR-2251-178 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 28] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 MR-2251-178 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 7 MR-2251-178 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ MR-2251-178 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD MR-2251-178 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G MR-2251-178 3 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G MR-2251-178 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MR-2251-178 5 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G MR-2251-178 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G MR-2251-178 7 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 29] Visit: 13 (7A) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-7469 COS/FUV ACQ/PEA PSA G130M 1291 1 5 S (5 S) KXD Comments: Exposure time is chosen for the faintest historical flux, 1.2e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-7469 COS/FUV ACQ/PEA PSA G130M 1291 NUM-POS=5, STEP-SIZE=0.9, 1 5 S (5 S) KD CENTER=FLUX-WT-FLR Comments: Exposure time is chosen for the faintest historical flux, 1.2e-14. ------------------------------------------------------------------------------------------------------------------------------------ 3 NGC-7469 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=311, FP-POS=ALL 1 421 S G (1684 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 NGC-7469 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 NGC-7469 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 6 NGC-7469 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 15673( 2) - 08-Jan-2019 13:11:41 - [ 30] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ 7 NGC-7469 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-7469 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD NGC-7469 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G NGC-7469 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-7469 5 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-7469 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G NGC-7469 7 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 31] Visit: 14 (7B) Visit Requirements: SCHED 100%; ON HOLD ; TOO RESPONSE TIME 14.0D On Hold Comments: This visit is on hold until the TOO is triggered. Additional Comments: This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 NGC-7469 COS/FUV ACQ/PEA PSA G130M 1291 1 5 S (5 S) KXD Comments: Exposure time is chosen for the faintest historical flux, 1.2e-14. ------------------------------------------------------------------------------------------------------------------------------------ 2 NGC-7469 COS/FUV ACQ/PEA PSA G130M 1291 NUM-POS=5, STEP-SIZE=0.9, 1 5 S (5 S) KD CENTER=FLUX-WT-FLR Comments: Exposure time is chosen for the faintest historical flux, 1.2e-14. ------------------------------------------------------------------------------------------------------------------------------------ 3 NGC-7469 COS/FUV TIME-TA PSA G130M 1222 BUFFER-TIME=311, FP-POS=ALL 1 421 S G (1684 S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 4 NGC-7469 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=3 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 5 NGC-7469 COS/FUV TIME-TA PSA G160M 1533 BUFFER-TIME=370, FP-POS=4 1 480 S (480 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 15673( 2) - 08-Jan-2019 13:11:41 - [ 32] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 NGC-7469 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=1 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ 7 NGC-7469 COS/FUV TIME-TA PSA G160M 1623 BUFFER-TIME=454, FP-POS=2 1 564 S (564 G S) Comments: We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ NGC-7469 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD NGC-7469 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 1 1 N/A G NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 2 1 N/A G NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 3 1 N/A G NGC-7469 3 COS/FUV TIME-TA PSA G130M 1222 none none none 4 1 N/A G NGC-7469 4 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-7469 5 COS/FUV TIME-TA PSA G160M 1533 none none none none 2 N/A G NGC-7469 6 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G NGC-7469 7 COS/FUV TIME-TA PSA G160M 1623 none none none none 2 N/A G 15673( 2) - 08-Jan-2019 13:11:41 - [ 33] Summary Form for Proposal 15673 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures PSA ------------------------------------------------------------------------------------------------------------------------------------ Configurations COS/FUV, COS/NUV ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACQ/IMAGE, ACQ/PEAKD, ACQ/PEAKXD, TIME-TAG ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters BUFFER-TIME=300, BUFFER-TIME=3000, BUFFER-TIME=309, BUFFER-TIME=311, BUFFER-TIME=355, BUFFER-TIME=358, BUFFER-TIME=361, BUFFER-TIME=370, BUFFER-TIME=454, CENTER=FLUX-WT-FLR, FP-POS=1, FP-POS=2, FP-POS=3, FP-POS=4, FP-POS=ALL, NUM-POS=5, STEP-SIZE=0.9 ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements ON HOLD , SCHED 100%, TOO RESPONSE TIME 14.0D ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements G130M, G160M, MIRRORB ------------------------------------------------------------------------------------------------------------------------------------ Target Names ARK-564, MR-2251-178, MRK-509, MRK-841, NGC-3227, NGC-4593, NGC-7469 ------------------------------------------------------------------------------------------------------------------------------------