15675( 12) - 10-Apr-2019 14:55:11 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 15675 Version: 12 Check-in Time: 10-Apr-2019 14:55:11 STScI Edit Number: 6 Title A New Approach to Following Transients with HST: Rolling Snapshots ------------------------------------------------------------------------------------ Type Cycle SNAP 26 ------------------------------------------------------------------------------------ Investigators Contact? PI: Dr. Andrew S. Fruchter Space Telescope Science Institute Y CoI: Dr. David Rubin Space Telescope Science Institute N CoI: Mr. Kishalay De California Institute of Technology N CoI: Dr. Mansi Kasliwal California Institute of Technology N ------------------------------------------------------------------------------------ Abstract We are now entering an era in which large scale surveys of the sky will discover numerous transients each night. The number of targets that could benefit from HST observations on timescales of less than three weeks will easily exceed the ability of HST to schedule disruptive ToO observations. Here we propose a variant of snapshot scheduling that would allow transients to be observed as soon as 11 days after discovery with little to no additional overhead compared to a standard snapshot program. We call this new observational approach ``Rolling Snapshots.'' While any one object will have a low probability of being observed in such a program, the large number of transients available will make it possible to build up statistically significant samples, with the the type of transient and exact observation scheme determined by the science under investigation. Here we ask to use rolling snapshots to obtain WFC3 UV grism spectra of a limited sample of Type Ia, Type II and superluminous supernovae discovered by the Zwicky Transient Facility. This program will allow us to verify that Rolling Snapshots are indeed an efficient use of obsevatory resources and will also give a taste of some of the exciting science the community could undertake with Rolling Snapshots. ------------------------------------------------------------------------------------ Observations Description ------------------------ In this test program, we are using the WFC3/UVIS grism to obtain UV spectra of transients shortly after outburst. We will use the G280Lgrism and take spectra of 500 seconds (split into two dithers). We will also obtain F350LP images of the field. These images have two purposes. First they will serve as the reference image allowing us to set the wavelength scale of the spectra. However, we expect that in over twenty-five percent of our images the first order spectrum of the transient will land on the zeroth order spectrum of the host galaxy in a region where the zeroth order spectrum is bright enough to contribute noticeable contamination. The F350LP filter has very similar throughput to the zeroth order of the G280 grism. We wish to also test whether subtraction of the F350LP image from first order spectrum can be used to reduce this contamination. We are using a custom 1024x1024 subarray in order to reduce readout overhead and buffer dumps to decrease the total time used. We need a custom subarray as the G280 can only be used with the UVIS aperture. 15675( 12) - 10-Apr-2019 14:55:11 - [ 2] ------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 3] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 11 ZTF19AAINJPZ EXT-STAR, SUPERNOVA, RA=04H19M58.1000S +/- 1", J2000 V = 19 +/- 4 SUPERNOVA TYPE IA DEC=-07D15'24.50" +/- 1" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 13 AT2019ABN STAR, SUPERNOVA RA=13H29M42.4000S, J2000 V = 18 DEC=+47D11'16.60" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 14 SN2019BKH EXT-STAR, SUPERNOVA, RA=13H08M57.3100S, J2000 V = 18 SUPERNOVA TYPE IA DEC=+28D16'51.90" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 15 SN2018IBB EXT-STAR, SUPERNOVA RA=04H38M56.9300S, J2000 V = 20 DEC=-20D39'44.20" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 16 SN2018LNB EXT-STAR, SUPERNOVA RA=10H38M32.7500S +/- 1", J2000 V = 18.5 DEC=+48D16'31.00" +/- 1" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 17 SN2019CMY EXT-STAR, SUPERNOVA RA=15H08M50.8400S +/- 1", J2000 V = 18 DEC=+40D42'49.50" +/- 1" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 18 ZTF18ABFCMJW EXT-STAR, SUPERNOVA RA=17H36M46.7419S +/- 0.2", J2000 V = 20 TYPE II DEC=+50D32'52.17" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 19 SN2019CVZ EXT-STAR, SUPERNOVA RA=16H30M54.0869S, J2000 V = 19 TYPE II DEC=+46D35'18.43" Reference Frame: ICRS ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 4] TARGET LIST Generic Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Selection Criteria | Flux data No | Name | Description | | ------------------------------------------------------------------------------------------------------------------------------------ 12 PLACEHOLDER- EXT-STAR, SUPERNOVA PI ACTIVATED V = 19.0 TARGET ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 5] Patterns ------------------------------------------------------------------------------------------------------------------------------------ Pattern_Number: 1 Primary_Pattern Secondary_Pattern Pattern_Type WFC3-UVIS-DITHER-LINE Pattern_Purpose DITHER Number_Of_Points 2 Point_Spacing 0.145 Line_Spacing Coordinate_Frame POS-TARG Pattern_Orient 46.84 Angle_Between_Sides Center_Pattern NO ------------------------------------------------------------------------------------------------------------------------------------ Pattern_Number: 2 Primary_Pattern Secondary_Pattern Pattern_Type WFC3-UVIS-DITHER-LINE Pattern_Purpose DITHER Number_Of_Points 2 Point_Spacing 0.145 Line_Spacing Coordinate_Frame POS-TARG Pattern_Orient 226.84 Angle_Between_Sides Center_Pattern NO ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 6] Visit: 3A Visit Requirements: BEFORE 18-MAR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 AT2019ABN WFC3/UVI ACCUM UVIS F275W SIZEAXIS1=1024, 1 200 S (400 POS TARG -61, -76; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 7] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 AT2019ABN WFC3/UVI ACCUM UVIS F336W SIZEAXIS1=1024, 1 150 S (300 POS TARG -61, -76; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 8] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 AT2019ABN WFC3/UVI ACCUM UVIS F814W SIZEAXIS1=1024, 1 75 S (150 POS TARG -61, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ AT2019ABN 1 WFC3/UVI ACCUM UVIS F275W 1 none none none 1 N/A S AT2019ABN 1 WFC3/UVI ACCUM UVIS F275W 2 none none none 1 N/A S AT2019ABN 2 WFC3/UVI ACCUM UVIS F336W 1 none none none 1 N/A S AT2019ABN 2 WFC3/UVI ACCUM UVIS F336W 2 none none none 1 N/A S AT2019ABN 3 WFC3/UVI ACCUM UVIS F814W 1 none none none 1 N/A S AT2019ABN 3 WFC3/UVI ACCUM UVIS F814W 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 9] Visit: 4A Visit Requirements: BEFORE 25-MAR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 SN2019BKH WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 50 S (100 POS TARG -61.22, -76.22; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 2 SN2019BKH WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61.22, -76.22; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 11] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 SN2019BKH WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -61, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ SN2019BKH 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S SN2019BKH 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S SN2019BKH 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S SN2019BKH 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S SN2019BKH 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S SN2019BKH 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 12] Visit: 5A Visit Requirements: BEFORE 21-APR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 SN2018IBB WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 30 S (60 POS TARG -61.22, -76.22; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 13] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 SN2018IBB WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61.22, -76.22; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 3 SN2018IBB WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -61, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ SN2018IBB 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S SN2018IBB 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S SN2018IBB 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S SN2018IBB 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S SN2018IBB 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S SN2018IBB 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 15] Visit: 5B Visit Requirements: BEFORE 07-APR-2019:00:00:00; ON HOLD On Hold Comments: This SN has been fading rapidly, so we are removing it from observation Additional Comments: This is for UVIS2, the preferred chip. 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 SN2018LNB WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 15 S (30 POS TARG -61.22, -76.22; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 2 SN2018LNB WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61.22, -76.22; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 17] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 SN2018LNB WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -61, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ SN2018LNB 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S SN2018LNB 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S SN2018LNB 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S SN2018LNB 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S SN2018LNB 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S SN2018LNB 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 18] Visit: 6A Visit Requirements: BEFORE 21-APR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 SN2019CMY WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 50 S (100 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 19] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 SN2019CMY WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 3 SN2019CMY WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -59, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -59" -76". ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ SN2019CMY 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S SN2019CMY 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S SN2019CMY 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S SN2019CMY 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S SN2019CMY 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S SN2019CMY 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 21] Visit: 6B Visit Requirements: BEFORE 21-APR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 SN2018IBB WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 30 S (60 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 2 SN2018IBB WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 23] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 SN2018IBB WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -59, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -59" -76". ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ SN2018IBB 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S SN2018IBB 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S SN2018IBB 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S SN2018IBB 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S SN2018IBB 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S SN2018IBB 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 24] Visit: 7A Visit Requirements: BEFORE 28-APR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 SN2019CMY WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 50 S (100 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 25] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 SN2019CMY WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 3 SN2019CMY WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -59, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -59" -76". ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ SN2019CMY 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S SN2019CMY 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S SN2019CMY 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S SN2019CMY 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S SN2019CMY 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S SN2019CMY 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 27] Visit: 7B Visit Requirements: BEFORE 28-APR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 ZTF18ABFCMJ WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 30 S (60 POS TARG -61, -80; W S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 2 ZTF18ABFCMJ WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61, -80; W S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 29] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 ZTF18ABFCMJ WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -59, -76; W S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -59" -76". ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ ZTF18ABFCMJW 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S ZTF18ABFCMJW 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S ZTF18ABFCMJW 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S ZTF18ABFCMJW 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S ZTF18ABFCMJW 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S ZTF18ABFCMJW 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 30] Visit: 7C Visit Requirements: BEFORE 28-APR-2019:00:00:00 On Hold Comments: Additional Comments: This is for UVIS2, the preferred chip. 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 SN2019CVZ WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 30 S (60 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 1 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 31] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 SN2019CVZ WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (500 POS TARG -61, -80; S SIZEAXIS2=1024, S) PATTERN 1 2 CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -61" -80". ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 3 SN2019CVZ WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (200 POS TARG -59, -76; S SIZEAXIS2=1024, S) PATTERN 1 3 CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. DR Note: Moving an additional 4" to better remove offset between F350LP and G280 to -59" -76". ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ SN2019CVZ 1 WFC3/UVI ACCUM UVIS F300X 1 none none none 1 N/A S SN2019CVZ 1 WFC3/UVI ACCUM UVIS F300X 2 none none none 1 N/A S SN2019CVZ 2 WFC3/UVI ACCUM UVIS G280 1 none none none 1 N/A S SN2019CVZ 2 WFC3/UVI ACCUM UVIS G280 2 none none none 1 N/A S SN2019CVZ 3 WFC3/UVI ACCUM UVIS F350LP 1 none none none 1 N/A S SN2019CVZ 3 WFC3/UVI ACCUM UVIS F350LP 2 none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 33] Visit: T1 Visit Requirements: ON HOLD On Hold Comments: Template for future visits. Additional Comments: This is for UVIS2, the preferred chip. 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 PLACEHOLDER WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 10 S (10 POS TARG -61.22, -76.22 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=513, FLASH=12 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 34] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 PLACEHOLDER WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (250 POS TARG -61.22, -76.22 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 35] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 PLACEHOLDER WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (250 POS TARG -61, -76 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=513 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 36] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 4 PLACEHOLDER WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (100 POS TARG -61, -76 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 37] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 5 PLACEHOLDER WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (100 POS TARG -61.22, -70.22 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=513, FLASH=5 Comments: We are effectively duplicating the UVIS2-C1K1C-SUB aperture, but using the UVIS aperture appropriate for G280. The nominal position is 537.0, 512.0 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, -72".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ PLACEHOLDER-TARGET 1 WFC3/UVI ACCUM UVIS F300X none none none none 1 N/A S PLACEHOLDER-TARGET 2 WFC3/UVI ACCUM UVIS G280 none none none none 1 N/A S PLACEHOLDER-TARGET 3 WFC3/UVI ACCUM UVIS G280 none none none none 1 N/A S PLACEHOLDER-TARGET 4 WFC3/UVI ACCUM UVIS F350LP none none none none 1 N/A S PLACEHOLDER-TARGET 5 WFC3/UVI ACCUM UVIS F350LP none none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 38] Visit: T2 Visit Requirements: ON HOLD On Hold Comments: Template for future visits. Additional Comments: This is for UVIS1, to be used only if UVIS2 won't schedule because of the large POSTARG. 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 PLACEHOLDER WFC3/UVI ACCUM UVIS F300X SIZEAXIS1=1024, 1 10 S (10 POS TARG -61.22, 49.22 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=1539, FLASH=12 Comments: The nominal position is 512.0, 3581 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, 49".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 39] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 PLACEHOLDER WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (250 POS TARG -61.22, 49.22 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=1539 Comments: The nominal position is 512.0, 3581 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, 49".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 3 PLACEHOLDER WFC3/UVI ACCUM UVIS G280 SIZEAXIS1=1024, 1 250 S (250 POS TARG -61, 49 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=1539 Comments: The nominal position is 512.0, 3581 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, 49".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 40] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 4 PLACEHOLDER WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (100 POS TARG -61, 49 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=1539, FLASH=5 Comments: The nominal position is 512.0, 3581 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, 49".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 5 PLACEHOLDER WFC3/UVI ACCUM UVIS F350LP SIZEAXIS1=1024, 1 100 S (100 POS TARG -61.22, 49.22 -TARGET S SIZEAXIS2=1024, S) CENTERAXIS1=515, CENTERAXIS2=1539, FLASH=5 Comments: The nominal position is 512.0, 3581 while for UVIS, it's 2073.0, 250.0 (or effectively 2073.0, 2332). So we want a POSTARG of -61".0, 49".0. This was slightly refined in Aladin. From SB: One minor comment I'd have is to consider shifting the area for the subarray readout slightly to the left, in order to include the left overscan i.e. decrease CENTERAXIS1 by 23. By including the overscan columns in the subarray, the calibration software can compute the correction using the image itself rather than using a default look-up value. Note: 23 not 25 is the number of overscan pixels for a subarray. New note: CENTERAXIS includes overscan, so use 513. DR note: 515 to stop the warnings. ------------------------------------------------------------------------------------------------------------------------------------ 15675( 12) - 10-Apr-2019 14:55:11 - [ 41] 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 | ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ PLACEHOLDER-TARGET 1 WFC3/UVI ACCUM UVIS F300X none none none none 1 N/A S PLACEHOLDER-TARGET 2 WFC3/UVI ACCUM UVIS G280 none none none none 1 N/A S PLACEHOLDER-TARGET 3 WFC3/UVI ACCUM UVIS G280 none none none none 1 N/A S PLACEHOLDER-TARGET 4 WFC3/UVI ACCUM UVIS F350LP none none none none 1 N/A S PLACEHOLDER-TARGET 5 WFC3/UVI ACCUM UVIS F350LP none none none none 1 N/A S 15675( 12) - 10-Apr-2019 14:55:11 - [ 42] Summary Form for Proposal 15675 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures UVIS ------------------------------------------------------------------------------------------------------------------------------------ Configurations WFC3/UVIS ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACCUM ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters CENTERAXIS1=515, CENTERAXIS2=1539, CENTERAXIS2=513, FLASH=12, FLASH=5, SIZEAXIS1=1024, SIZEAXIS2=1024 ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements BEFORE 07-APR-2019:00:00:00, BEFORE 18-MAR-2019:00:00:00, BEFORE 21-APR-2019:00:00:00, BEFORE 25-MAR-2019:00:00:00, BEFORE 28-APR-2019:00:00:00, ON HOLD , PATTERN 1 1, PATTERN 1 2, PATTERN 1 3, POS TARG -59, -76, POS TARG -61, -76, POS TARG -61, -80, POS TARG -61, 49, POS TARG -61.22, -70.22, POS TARG -61.22, -76.22, POS TARG -61.22, 49.22 ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements F275W, F300X, F336W, F350LP, F814W, G280 ------------------------------------------------------------------------------------------------------------------------------------ Target Names AT2019ABN, PLACEHOLDER-TARGET, SN2018IBB, SN2018LNB, SN2019BKH, SN2019CMY, SN2019CVZ, ZTF18ABFCMJW ------------------------------------------------------------------------------------------------------------------------------------