0Assigned ID: 930
----- Attempting Submission 1 (Fri Apr 08 22:38:41 GMT 2016) -----
HST Phase I Proposal 930 (K23d_K218d.apt) successfully submitted.
Receipt: # 930-1EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO
EXPOSURE WITH SAA CONTOUR 11 WILL EXECUTE ON GYRO0----- Attempting Submission 1 (Thu Jul 21 21:04:14 GMT 2016) -----
----- Attempting Submission 2 (Wed Aug 17 19:20:37 GMT 2016) -----
----- Attempting Submission 3 (Fri Oct 28 00:12:50 GMT 2016) -----
HST Phase II Proposal 14682 (HST_GO_14682_20161027_2.apt) successfully submitted.
Receipt: # 14682-3
----- Attempting Submission 4 (Sat Oct 29 22:51:42 GMT 2016) -----
HST Phase II Proposal 14682 (HST_GO_14682_20161029_v3.apt) successfully submitted.
Receipt: # 14682-4
----- Attempting Submission 5 (Wed Nov 02 00:17:57 GMT 2016) -----
----- Attempting Submission 6 (Fri Dec 09 22:14:48 GMT 2016) -----
----- Attempting Submission 7 (Tue Jan 17 16:44:36 GMT 2017) -----
----- Attempting Submission 8 (Tue Oct 24 20:28:28 GMT 2017) -----
----- Attempting Submission 9 (Mon Nov 20 23:20:34 GMT 2017) -----
----- Attempting Submission 10 (Wed Jan 24 06:05:05 GMT 2018) -----
----- Attempting Submission 11 (Tue Jan 30 15:35:37 GMT 2018) -----
HST Phase II Proposal 14682 (HST_GO_14682_20180130_v2.apt) successfully submitted.
Receipt: # 14682-11
----- Attempting Submission 12 (Tue Jan 30 19:42:23 GMT 2018) -----
----- Attempting Submission 13 (Tue Jan 30 20:14:26 GMT 2018) -----
----- Attempting Submission 14 (Tue Apr 03 19:07:48 GMT 2018) -----
----- Attempting Submission 15 (Tue Nov 20 05:22:20 GMT 2018) -----
HST Phase II Proposal 14682 (HST_GO_14682_20180403_modVisit12.apt) successfully submitted.
Receipt: # 14682-15
----- Attempting Submission 16 (Thu Dec 06 19:35:25 GMT 2018) -----There are warnings because we observe exposures in gyro control during SAA passage.A Search for Methane, Ammonia, and Water on Two Habitable Zone Super-EarthsThe recent discovery of two transiting super-Earths in the habitable zones of bright, nearby M-dwarfs provides us with the unprecedented opportunity to carry out the first spectroscopic studies of the atmospheres of potentially habitable planets outside our solar system. The planets' equilibrium temperatures of 210-275 K and 225-305 K, respectively, are consistent with the potential presence of liquid water, a condition generally regarded as a necessity for the existence of life as we know it. Here, we propose to obtain HST WFC3 transmission spectroscopy of both planets in order to infer their atmospheric hydrogen fractions, carbon-to-nitrogen ratios (C/N), and to determine their potential habitability. Our proposed observations will cleanly distinguish between cloud-free, H2-dominated scenarios and high mean molecular mass (e.g. H2O-dominated) atmospheres. For hydrogen-rich atmospheres we can determine the C/N ratio based on the relative strengths of methane and ammonia absorption, allowing us to distinguish between H2/He atmospheres accreted from the protoplanetary disk and H2-rich atmospheres formed through outgassing. The detection of absorption from methane, ammonia, and/or water will make K2-18b and K2-3d prime targets for first-light observations with JWST to search for biosignatures in their atmospheres. Observations in HST Cycle 24 will allow us to determine the atmospheric compositions and potential habitability of these planets prior to JWST Cycle 1 deadline.Our program observes two transits of HIP116454b using WFC3 G141 (1-1.7 micron) spectroscopyExtrasolar Planets and Planet Formation0falsefalsefalsefalsefalsefalsefalseAVAILABLESTARM III-IThis object was generated by the targetselector and retrieved from the 2MASS database.EPIC201367065DK2-3BJ2000J2000J = 9.421 +/- 0.027; H = 8.805 +/- 0.044STARM III-IEPIC201912552BK2-18DJ2000J2000J = 9.76; H = 9.13WFC3/IRSpectroscopicNoNoG141WFC3/IRSpectroscopicNoNoG141The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v01.xmlWFC3/G141 transit visit of K2-18b. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Six identical visits of K2-18b will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1483558749000278.29134753524664(Tic-Visit
:proposal-id 14682
:visit-id "01"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:12:49.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1810016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "01"
:obset-id "01"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "01"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2630
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "01"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "01"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "01"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "01"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 478
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)false50The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v02.xmlWFC3/G141 transit visit of K2-18b. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Six identical visits of K2-18b will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1486402903000286.954099776817(Tic-Visit
:proposal-id 14682
:visit-id "02"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:13:11.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1598768
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "02"
:obset-id "02"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "02"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2630
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "02"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "02"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2414
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "02"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2130
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "02"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 1988
:al-overhead-at-end 0
:internal-dur-at-end 436
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)false50The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v03.xmlWFC3/G141 transit visit of K2-18b. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Six identical visits of K2-18b will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1480708964000293.94790769741337(Tic-Visit
:proposal-id 14682
:visit-id "03"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:13:34.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1694784
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "03"
:obset-id "03"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "03"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2630
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "03"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "03"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "03"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2414
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "03"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2130
:al-overhead-at-end 0
:internal-dur-at-end 478
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)false50The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v04.xmlWFC3/G141 transit visit of K2-18b. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Six identical visits of K2-18b will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1492096664000123.52585901320572(Tic-Visit
:proposal-id 14682
:visit-id "04"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:13:59.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1810016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "04"
:obset-id "04"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "04"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2630
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "04"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "04"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "04"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "04"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 478
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)false50The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v05.xmlWFC3/G141 transit visit of K2-18b. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Six identical visits of K2-18b will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1512014730000294.16289441784113(Tic-Visit
:proposal-id 14682
:visit-id "05"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:14:18.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1464320
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "05"
:obset-id "05"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "05"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2630
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "05"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "05"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "05"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 1420
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "05"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 1420
:al-overhead-at-end 0
:internal-dur-at-end 478
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)false50The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v06.xmlWFC3/G141 transit visit of K2-18b. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Six identical visits of K2-18b will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1526243665000132.0(Tic-Visit
:proposal-id 14682
:visit-id "06"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:14:43.0"
:trans-errors '(:WARNINGS 8 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1752400
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "06"
:obset-id "06"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "06"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2488
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "06"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "06"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "06"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "06"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2435
:al-overhead-at-end 0
:internal-dur-at-end 478
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2982
:pcs-gap 0
)false50The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v07.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1483850609000297.0(Tic-Visit
:proposal-id 14682
:visit-id "07"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:15:16.0"
:trans-errors '(:WARNINGS 10 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2174928
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "07"
:obset-id "07"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "07"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2632
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "07"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "07"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "07"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "07"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "07"
:orbit-number 6
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 436
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)false60The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v08.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1479999207000291.6082063743419(Tic-Visit
:proposal-id 14682
:visit-id "08"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:15:47.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2021280
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "08"
:obset-id "08"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "08"
:orbit-number 1
:pcs-time 241
:si-vis-utilization 1780
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "08"
:orbit-number 2
:pcs-time 176
:si-vis-utilization 2414
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "08"
:orbit-number 3
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "08"
:orbit-number 4
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "08"
:orbit-number 5
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "08"
:orbit-number 6
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 457
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)false60The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v09.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1487701975000315.505763649609(Tic-Visit
:proposal-id 14682
:visit-id "09"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:16:19.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2174928
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "09"
:obset-id "09"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "09"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2632
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "09"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "09"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "09"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "09"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "09"
:orbit-number 6
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 436
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)false60The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v10.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1491547247000103.49873581633727(Tic-Visit
:proposal-id 14682
:visit-id "10"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:16:53.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2174928
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "10"
:obset-id "10"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "10"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2632
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "10"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "10"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "10"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "10"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "10"
:orbit-number 6
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 436
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)false60The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v11.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1510796067000290.7739803276517(Tic-Visit
:proposal-id 14682
:visit-id "11"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:17:28.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2166512
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "11"
:obset-id "11"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "11"
:orbit-number 1
:pcs-time 241
:si-vis-utilization 2632
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "11"
:orbit-number 2
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "11"
:orbit-number 3
:pcs-time 176
:si-vis-utilization 2647
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "11"
:orbit-number 4
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "11"
:orbit-number 5
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "11"
:orbit-number 6
:pcs-time 176
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 478
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)false60The scheduling data was generated by CASM 26.2.2.CASM was run in Phase II mode./private/var/folders/21/j6tc2nwn69b30pd1dyh301cr0000gn/T/OPVisit3420613278836979534.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).(Tic-Visit
:proposal-id 14682
:visit-id "12"
:proposal-version -1
:trans-version "20181130"
:date "06-Dec-2018 14:34:21.0"
:trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 1944464
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "12"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2064
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "12"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2130
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "12"
:orbit-number 3
:pcs-time 302
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "12"
:orbit-number 4
:pcs-time 302
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "12"
:orbit-number 5
:pcs-time 302
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "12"
:orbit-number 6
:pcs-time 302
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 436
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true60The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v13.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1514646448000315.531736400056(Tic-Visit
:proposal-id 14682
:visit-id "13"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:18:04.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2117312
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "13"
:obset-id "13"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "13"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2632
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "13"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "13"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "13"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "13"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2556
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "13"
:orbit-number 6
:pcs-time 222
:si-vis-utilization 2414
:al-overhead-at-end 0
:internal-dur-at-end 436
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)false60The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./Users/bbenneke/Research/Proposals_for_Observations/26_HST_Cycle24_Proposal_Two_HZ_SuperEarths/OP-cache/HST_GO_14682_20180403_modVisit12_secondTime-v14.xmlWFC3/G141 transit visit of K2-3d. It is essential for the orbits in each visit to be scheduled in a contiguous block.
Eight identical visits of K2-3d will be taken to build up the required SNR.
The repeated observations and the relatively long orbital period of this habitable zone planet may present a challenge in the scheduling process. If beneficial for the scheduling, please feel free to observe the target with only one guide star. We have successfully done this for the bright star HD97658b in program GO 13501 (Knutson et al. 2014b). Also, if necessary, feel free to observe during the SAA passage. A contiguous block of >10 orbits to measure the phase curve of WASP-43b using WFC3 did not show any significant negative effects on the data quality for transit spectroscopy (Stevenson et al., 2014).1518497284000315.5321729358802(Tic-Visit
:proposal-id 14682
:visit-id "14"
:proposal-version -1
:trans-version "20180409"
:date "20-Nov-2018 00:18:38.0"
:trans-errors '(:WARNINGS 6 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2155712
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14682
:visit-id "14"
:obset-id "14"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 14682
:visit-id "14"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2511
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "14"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "14"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "14"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "14"
:orbit-number 5
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14682
:visit-id "14"
:orbit-number 6
:pcs-time 222
:si-vis-utilization 2698
:al-overhead-at-end 0
:internal-dur-at-end 478
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2978
:pcs-gap 0
)false60