0 Assigned ID: 354 ----- Attempting Submission 1 (Fri Apr 11 03:43:51 GMT 2014) ----- HST Phase I Proposal 354 (super_earths_v1.apt) successfully submitted. ----- Attempting Submission 2 (Fri Apr 11 19:04:05 GMT 2014) ----- HST Phase I Proposal 354 (super_earths_v1.apt) successfully submitted. ----- Attempting Submission 3 (Fri Apr 11 22:49:07 GMT 2014) ----- HST Phase I Proposal 354 (super_earths_v1.apt) successfully submitted. ----- Attempting Submission 4 (Fri Apr 11 23:32:27 GMT 2014) ----- HST Phase I Proposal 354 (super_earths_v1.apt) successfully submitted. ----- Attempting Submission 5 (Fri Apr 11 23:55:08 GMT 2014) ----- 0 ----- Attempting Submission 1 (Thu Jul 24 17:13:20 GMT 2014) ----- HST Phase II Proposal 13665 (HST_GO_13665_phase2_v28_EarlySubmission.apt) successfully submitted. ----- Attempting Submission 2 (Thu Jul 24 23:42:00 GMT 2014) ----- Exploring the Diversity of Exoplanet Atmospheres in the Super-Earth Regime Super-Earths are the single most common type of extrasolar planet, and also one of the least well-understood. We expect these planets could form with a broad range of bulk compositions, including true "super-Earths" with primarily rocky interiors, "water worlds" with a supercritical interior surrounded by a steam atmosphere, and "mini-Neptunes" with a thick hydrogen and helium atmosphere surrounding a rocky or icy core. In this proposal we focus on five planets with masses ranging from that of Neptune down to that of the Earth, and use a combination of visible-light and near-IR transmission spectroscopy to constrain their atmopsheric compositions and resolve degeneracies in their corresponding interior compositions. Our observations will probe the poorly understood transition region between gas giant planets and terrestrial worlds and provide the first detailed look at the diversity (or lack thereof) of planets in this mass range. These same data will also enable the first detailed studies of cloud properties in these atmospheres, which can dramatically alter their atmospheric temperatures and corresponding compositions. The proposed studies will pave the way for future observations of this class of planets with JWST. Our program observes transits of five extrasolar planets using two different observing modes: WFC3 G141 (1-1.7 micron) spectroscopy, and STIS G750L (0.5-1 micron) spectroscopy. Each system is observed in visits of either 4 or 5 contiguous orbits. Note that we observe Kepler-138 only with WFC3 (no STIS) and we observe GJ436 only with STIS (no WFC3). It is essential for the orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. In order to ensure complete coverage of the transit light curve, each targets' visits have been scheduled with different offsets, corresponding to narrow, independent chunks of the desired visibility window. However, if this strategy poses a significant barrier to scheduling the requirements for individual visits may be relaxed to the full range (in orbital phase) specified for a given target. For STIS, we disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. GO12473 (PI Sing). We also intentionally oversaturate the STIS CCD with our observations of 55 Cancri and HD97658; this approach lets us achieve higher observing efficiency and has been successfully demonstrated in past programs, e.g. GO13180 (PI Ehrenreich). For WFC3, .... EXTRA-SOLAR PLANETS 12 false false false false false false AVAILABLE STAR EXTRA-SOLAR PLANETARY SYSTEM K V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 R=7.3, I=6.8, J=6.2, H=5.8 STAR EXTRA-SOLAR PLANETARY SYSTEM M V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 R=11.2, I=9.8, J=8.79, H=8.21 STAR EXTRA-SOLAR PLANETARY SYSTEM M V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 R=9.6, I=8.2, J=6.9, H=6.32 STAR EXTRA-SOLAR PLANETARY SYSTEM G V-IV K V-IV This star is in a double system (common proper motions) with 55 Cancri B (GJ 324B), a much fainter (V=13) M4 dwarf that is 1.4-arcmin away. It also 4.6-arcmin away from the similarly bright (V=6.3) star 53 Cancri (BO Cancri). HR3522 GJ324A J2000 B=6.82, R=5.4, I=5.0, J=4.768, H=4.265, K=4.015 STAR EXTRA-SOLAR PLANETARY SYSTEM M V-IV Additional data were added to this entry by hand. Fluxes were converted from SDSS magnitudes in the Kepler Input Catalog. This object was generated by the targetselector and retrieved from the SIMBAD database. 2MASS-J19213157+4317347 J2000 R=12.7, I=12.0, J=10.3, H=9.7 STAR M III-I J2000 J2000 J = 9.76; H = 9.13 STAR K III-I This object was generated by the targetselector and retrieved from the SIMBAD database. Refined by Benneke. J2000 U=7.46, B=6.56, R=4.76, J=3.86, H=3.40, K=3.25 STIS/CCD Spectroscopic No No G750L 7751 WFC3/IR Spectroscopic No No G141 STIS/CCD Spectroscopic No No G750L 7751 WFC3/IR Spectroscopic No No G141 STIS/CCD Spectroscopic No No G750L 7751 STIS/CCD Spectroscopic No No G750L 7751 WFC3/IR Spectroscopic No No G141 WFC3/IR Spectroscopic No No G141 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of six) WFC3/G141 transit visits of Kepler 138 It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each Kepler-138 visit observe Kepler-138 during the transit of Kepler-138c. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9915-0.9924 in planet orbital phase, corresponding to a 27 minute interval. In order to also ensure complete coverage of the transit light curve when combining the six visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second one has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to the full 27 minute range (0.9915-0.9924) in orbital phase. We also included orientation restrictions intended to avoid overlapping spectra with nearby stars. Kepler 138 is in a very crowded field of the sky. 1419126301000 17.0 (Tic-Visit :proposal-id 13665 :visit-id "01" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:43:56.0" :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 13665 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of six) WFC3/G141 transit visits of Kepler 138 We also included orientation restrictions intended to avoid overlapping spectra with nearby stars. Kepler 138 is in a very crowded field of the sky. Can be relaxed if necessary 1445061040000 80.0 (Tic-Visit :proposal-id 13665 :visit-id "02" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:44:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1445120 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "02" :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "02" :orbit-number 4 :pcs-time 222 :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 2991 :pcs-gap 0 ) false 4 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Thrid (of six) WFC3/G141 transit visits of Kepler 138 It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each Kepler-138 visit observe Kepler-138 during the transit of Kepler-138c. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9915-0.9924 in planet orbital phase, corresponding to a 27 minute interval. In order to also ensure complete coverage of the transit light curve when combining the six visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second one has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to the full 27 minute range (0.9915-0.9924) in orbital phase. We also included orientation restrictions intended to avoid overlapping spectra with nearby stars. Kepler 138 is in a very crowded field of the sky. 1429100982000 260.0 (Tic-Visit :proposal-id 13665 :visit-id "03" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:44:54.0" :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 13665 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "03" :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "03" :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 2991 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Fourth (of six) WFC3/G141 transit visits of Kepler 138 It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each Kepler-138 visit observe Kepler-138 during the transit of Kepler-138c. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9915-0.9924 in planet orbital phase, corresponding to a 27 minute interval. In order to also ensure complete coverage of the transit light curve when combining the six visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second one has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to the full 27 minute range (0.9915-0.9924) in orbital phase. We also included orientation restrictions intended to avoid overlapping spectra with nearby stars. Kepler 138 is in a very crowded field of the sky. (Tic-Visit :proposal-id 13665 :visit-id "04" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:45:26.0" :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 13665 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Fifth (of six) WFC3/G141 transit visits of Kepler 138 It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each Kepler-138 visit observe Kepler-138 during the transit of Kepler-138c. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9915-0.9924 in planet orbital phase, corresponding to a 27 minute interval. In order to also ensure complete coverage of the transit light curve when combining the six visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second one has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to the full 27 minute range (0.9915-0.9924) in orbital phase. We also included orientation restrictions intended to avoid overlapping spectra with nearby stars. Kepler 138 is in a very crowded field of the sky. (Tic-Visit :proposal-id 13665 :visit-id "05" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:48:49.0" :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 13665 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2629 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "05" :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "05" :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 2991 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Sixth (of six) WFC3/G141 transit visits of Kepler 138 It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each Kepler-138 visit observe Kepler-138 during the transit of Kepler-138c. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9915-0.9924 in planet orbital phase, corresponding to a 27 minute interval. In order to also ensure complete coverage of the transit light curve when combining the six visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second one has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to the full 27 minute range (0.9915-0.9924) in orbital phase. We also included orientation restrictions intended to avoid overlapping spectra with nearby stars. Kepler 138 is in a very crowded field of the sky. (Tic-Visit :proposal-id 13665 :visit-id "06" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:49:28.0" :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 13665 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2629 :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "06" :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "06" :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "06" :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 2991 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "06" :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 2991 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of four) STIS/G750L transit of HD 97658 b. These observations are designed to oversaturate the STIS CCD by a factor of ~2. Liberated charges will bleed along detector columns, but we will add up the "leaked" charge and recover all photoelectrons. It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each HD97658 STIS visit observe HD97658 during the transit of HD97658b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9794-0.9819 in planet orbital phase, corresponding to a 34 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.9794-0.9819 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9794-0.9819 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1430932162000 123.93496738795511 (Tic-Visit :proposal-id 13665 :visit-id "07" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:49:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 5 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 971776 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2636 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "07" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "07" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "07" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "07" :orbit-number 5 :pcs-time 222 :si-vis-utilization 2736 :al-overhead-at-end 120 :internal-dur-at-end 680 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 5 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of four) STIS/G750L transit of HD 97658 b. These observations are designed to oversaturate the STIS CCD by a factor of ~2. Liberated charges will bleed along detector columns, but we will add up the "leaked" charge and recover all photoelectrons. It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each HD97658 STIS visit observe HD97658 during the transit of HD97658b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9794-0.9819 in planet orbital phase, corresponding to a 34 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.9794-0.9819 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9794-0.9819 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). (Tic-Visit :proposal-id 13665 :visit-id "08" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:50:23.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 5 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 971776 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2636 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "08" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "08" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "08" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "08" :orbit-number 5 :pcs-time 222 :si-vis-utilization 2736 :al-overhead-at-end 120 :internal-dur-at-end 680 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 5 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Third (of four) STIS/G750L transit of HD 97658 b. These observations are designed to oversaturate the STIS CCD by a factor of ~2. Liberated charges will bleed along detector columns, but we will add up the "leaked" charge and recover all photoelectrons. It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each HD97658 STIS visit observe HD97658 during the transit of HD97658b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9794-0.9819 in planet orbital phase, corresponding to a 34 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.9794-0.9819 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9794-0.9819 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1435851870000 99.0 (Tic-Visit :proposal-id 13665 :visit-id "09" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:50:53.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 5 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 971776 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2636 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "09" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "09" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "09" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "09" :orbit-number 5 :pcs-time 222 :si-vis-utilization 2736 :al-overhead-at-end 120 :internal-dur-at-end 680 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 5 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Fourth (of four) STIS/G750L transit of HD 97658 b. These observations are designed to oversaturate the STIS CCD by a factor of ~2. Liberated charges will bleed along detector columns, but we will add up the "leaked" charge and recover all photoelectrons. It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each HD97658 STIS visit observe HD97658 during the transit of HD97658b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9794-0.9819 in planet orbital phase, corresponding to a 34 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.9794-0.9819 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9794-0.9819 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1435032998000 106.81753863522891 (Tic-Visit :proposal-id 13665 :visit-id "10" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:51:23.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 5 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 971776 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2636 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "10" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "10" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "10" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2736 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "10" :orbit-number 5 :pcs-time 222 :si-vis-utilization 2736 :al-overhead-at-end 120 :internal-dur-at-end 680 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 5 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of two) WFC3/G141 transit visits of HD 97658 b. It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each HD97658 STIS visit observe HD97658 during the transit of HD97658b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9794-0.9819 in planet orbital phase, corresponding to a 34 minute interval. In order to also ensure complete coverage of the transit light curve when combining these visits with previously taken data, the first visit has been scheduled to begin within the first 10 minutes of the phase windows. The second visit can be arbitrarilty placed within the entire 0.9794-0.9819 phase window. If the first visit places a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9794-0.9819 phase range. 1460447929000 140.6812419376874 (Tic-Visit :proposal-id 13665 :visit-id "11" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:52:36.0" :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 2949136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "11" :orbit-number 1 :pcs-time 241 :si-vis-utilization 2650 :al-overhead-at-end 0 :internal-dur-at-end 752 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "11" :orbit-number 2 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 757 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "11" :orbit-number 3 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 757 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "11" :orbit-number 4 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 757 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "11" :orbit-number 5 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 727 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of two) WFC3/G141 transit visits of HD 97658 b. It is essential for the five orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 and 4 in each HD97658 STIS visit observe HD97658 during the transit of HD97658b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9794-0.9819 in planet orbital phase, corresponding to a 34 minute interval. In order to also ensure complete coverage of the transit light curve when combining these visits with previously taken data, the first visit has been scheduled to begin within the first 10 minutes of the phase windows. The second visit can be arbitrarilty placed within the entire 0.9794-0.9819 phase window. If the first visit places a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9794-0.9819 phase range. (Tic-Visit :proposal-id 13665 :visit-id "12" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:53:53.0" :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 2949136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "12" :orbit-number 1 :pcs-time 241 :si-vis-utilization 2650 :al-overhead-at-end 0 :internal-dur-at-end 752 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "12" :orbit-number 2 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 757 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "12" :orbit-number 3 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 757 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "12" :orbit-number 4 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 757 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "12" :orbit-number 5 :pcs-time 176 :si-vis-utilization 2759 :al-overhead-at-end 0 :internal-dur-at-end 727 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 5 0 Phase windows are not calculated when the gap between schedulable intervals is less than 1 days, assuming no scheduling restrictions for constraint Phase 0.773/0.783. The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of four) STIS/G750L transit of 55 Cancri e. These observations are designed to oversaturate the STIS CCD by a factor of ~7. Liberated charges will bleed along detector columns, but we will add up the "leaked" charge and recover all photoelectrons. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each 55 Cnc STIS visit observes 55 Cnc during the transit of 55 Cnc e. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.7732-0.8194 in planet orbital phase, corresponding to a 49 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four STIS visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.7732-0.8194 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.7732-0.8194 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1414704222000 286.153343315101 (Tic-Visit :proposal-id 13665 :visit-id "13" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:54:15.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 2449648 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2666 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "13" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2726 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "13" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2726 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "13" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2726 :al-overhead-at-end 120 :internal-dur-at-end 677 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 1 Explicit WAVECAL, auto-waves disabled Phase windows are not calculated when the gap between schedulable intervals is less than 1 days, assuming no scheduling restrictions for constraint Phase 0.783/0.809. The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of four) STIS/G750L transit of 55 Cancri e. IIt is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each 55 Cnc STIS visit observes 55 Cnc during the transit of 55 Cnc e. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.7732-0.8194 in planet orbital phase, corresponding to a 49 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.7732-0.8194 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.7732-0.8194 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1431252355000 103.94457260897212 (Tic-Visit :proposal-id 13665 :visit-id "14" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:54:36.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1657488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2666 :al-overhead-at-end 0 :internal-dur-at-end 58 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "14" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2753 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "14" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2753 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "14" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2753 :al-overhead-at-end 120 :internal-dur-at-end 673 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 1 Explicit WAVECAL, auto-waves disabled Phase windows are not calculated when the gap between schedulable intervals is less than 1 days, assuming no scheduling restrictions for constraint Phase 0.773/0.819. The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Third (of four) STIS/G750L transit of 55 Cancri e. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each 55 Cnc STIS visit observes 55 Cnc during the transit of 55 Cnc e. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.7732-0.8194 in planet orbital phase, corresponding to a 49 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.7732-0.8194 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.7732-0.8194 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1432271712000 101.68559615636582 (Tic-Visit :proposal-id 13665 :visit-id "15" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:54:58.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1657488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "15" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2666 :al-overhead-at-end 0 :internal-dur-at-end 58 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "15" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2753 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "15" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2753 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "15" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2753 :al-overhead-at-end 120 :internal-dur-at-end 673 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 1 Explicit WAVECAL, auto-waves disabled Phase windows are not calculated when the gap between schedulable intervals is less than 1 days, assuming no scheduling restrictions for constraint Phase 0.773/0.783. The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of four) WFC3/G141 transit visits of 55 Cnc e. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each 55 Cnc STIS visit observes 55 Cnc during the transit of 55 Cnc e. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.7732-0.8194 in planet orbital phase, corresponding to a 49 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four WFC3 visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.7732-0.8194 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.7732-0.8194 phase range. 1450023387000 276.40203748315116 (Tic-Visit :proposal-id 13665 :visit-id "17" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:55:28.0" :trans-errors '(:WARNINGS 143 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2331136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "17" :obset-id "A7" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "17" :obset-id "B7" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "17" :obset-id "C7" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "17" :orbit-number 1 :pcs-time 241 :si-vis-utilization 2580 :al-overhead-at-end 0 :internal-dur-at-end 752 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "17" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "17" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "17" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 717 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 3 Phase windows are not calculated when the gap between schedulable intervals is less than 1 days, assuming no scheduling restrictions for constraint Phase 0.810/0.819. The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of four) WFC3/G141 transit visits of 55 Cnc e. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each 55 Cnc STIS visit observes 55 Cnc during the transit of 55 Cnc e. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.7732-0.8194 in planet orbital phase, corresponding to a 49 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four WFC3 visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.7732-0.8194 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.7732-0.8194 phase range. (Tic-Visit :proposal-id 13665 :visit-id "18" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:55:56.0" :trans-errors '(:WARNINGS 143 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2331136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "18" :obset-id "A8" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "18" :obset-id "B8" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "18" :obset-id "C8" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "18" :orbit-number 1 :pcs-time 241 :si-vis-utilization 2580 :al-overhead-at-end 0 :internal-dur-at-end 752 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "18" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "18" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "18" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 717 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 3 Phase windows are not calculated when the gap between schedulable intervals is less than 1 days, assuming no scheduling restrictions for constraint Phase 0.773/0.819. The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Thrid (of four) WFC3/G141 transit visits of 55 Cnc e. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each 55 Cnc STIS visit observes 55 Cnc during the transit of 55 Cnc e. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.7732-0.8194 in planet orbital phase, corresponding to a 49 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four WFC3 visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.7732-0.8194 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.7732-0.8194 phase range. 1443215638000 293.3597384587222 (Tic-Visit :proposal-id 13665 :visit-id "19" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:59:26.0" :trans-errors '(:WARNINGS 143 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2331136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "19" :obset-id "A9" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "19" :obset-id "B9" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "19" :obset-id "C9" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "19" :orbit-number 1 :pcs-time 241 :si-vis-utilization 2580 :al-overhead-at-end 0 :internal-dur-at-end 752 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "19" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "19" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "19" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 717 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 3 Phase windows are not calculated when the gap between schedulable intervals is less than 1 days, assuming no scheduling restrictions for constraint Phase 0.773/0.819. The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Fourth (of four) WFC3/G141 transit visits of 55 Cnc e. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each 55 Cnc STIS visit observes 55 Cnc during the transit of 55 Cnc e. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.7732-0.8194 in planet orbital phase, corresponding to a 49 minute interval. In order to also ensure complete coverage of the transit light curve when combining the four WFC3 visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows.. The remaining visits can be arbitrarilty placed within the entire 0.7732-0.8194 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.7732-0.8194 phase range. (Tic-Visit :proposal-id 13665 :visit-id "20" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 20:59:56.0" :trans-errors '(:WARNINGS 143 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2331136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "20" :obset-id "A0" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "20" :obset-id "B0" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13665 :visit-id "20" :obset-id "C0" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "20" :orbit-number 1 :pcs-time 241 :si-vis-utilization 2580 :al-overhead-at-end 0 :internal-dur-at-end 752 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "20" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "20" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 747 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "20" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2776 :al-overhead-at-end 0 :internal-dur-at-end 717 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 3 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of three) STIS/G750L transit of GJ 3470b. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-3470 STIS visit observes GJ-3470 during the transit of GJ-3470b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9515-0.9580 in planet orbital phase, corresponding to a 31 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three STIS visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire 0.9515-0.9580 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9515-0.9580 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1459657809000 100.07270900783999 (Tic-Visit :proposal-id 13665 :visit-id "21" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:01:58.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 259408 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "21" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2454 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "21" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2754 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "21" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2754 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "21" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2754 :al-overhead-at-end 120 :internal-dur-at-end 675 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2992 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of three) STIS/G750L transit of GJ 3470b. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-3470 STIS visit observes GJ-3470 during the transit of GJ-3470b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9515-0.9580 in planet orbital phase, corresponding to a 31 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three STIS visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire 0.9515-0.9580 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9515-0.9580 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1423335150000 76.49960164154652 (Tic-Visit :proposal-id 13665 :visit-id "22" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:02:01.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 259408 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "22" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2454 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "22" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2754 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "22" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2754 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "22" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2754 :al-overhead-at-end 120 :internal-dur-at-end 675 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2992 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Third (of three) STIS/G750L transit of GJ 3470b. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-3470 STIS visit observes GJ-3470 during the transit of GJ-3470b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9515-0.9580 in planet orbital phase, corresponding to a 31 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three STIS visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire 0.9515-0.9580 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9515-0.9580 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1431407012000 103.50512115485162 (Tic-Visit :proposal-id 13665 :visit-id "23" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:02:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 259408 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "23" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2454 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "23" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2754 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "23" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2754 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "23" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2754 :al-overhead-at-end 120 :internal-dur-at-end 675 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2992 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of three) WFC3/G141 transit visits of GJ-3470. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-3470 WFC3 visit observes GJ-3470 during the transit of GJ-3470b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9515-0.9580 in planet orbital phase, corresponding to a 31 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three WFC3 visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire 0.9515-0.9580 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9515-0.9580 phase range. 1426217039000 86.7103099075797 (Tic-Visit :proposal-id 13665 :visit-id "24" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:02:27.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1445120 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "24" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2633 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "24" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "24" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "24" :orbit-number 4 :pcs-time 222 :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 2992 :pcs-gap 0 ) false 4 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of three) WFC3/G141 transit visits of GJ-3470. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-3470 WFC3 visit observes GJ-3470 during the transit of GJ-3470b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9515-0.9580 in planet orbital phase, corresponding to a 31 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three WFC3 visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire 0.9515-0.9580 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9515-0.9580 phase range. 1445534237000 281.4409885802679 (Tic-Visit :proposal-id 13665 :visit-id "25" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:02:49.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1445120 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "25" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2633 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "25" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "25" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "25" :orbit-number 4 :pcs-time 222 :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 2992 :pcs-gap 0 ) false 4 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Third (of three) WFC3/G141 transit visits of GJ-3470. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-3470 WFC3 visit observes GJ-3470 during the transit of GJ-3470b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9515-0.9580 in planet orbital phase, corresponding to a 31 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three WFC3 visits, the first visit has been scheduled to begin within the first 10 minutes of the phase windows and the second visit has been scheduled to begin in the last 10 min of the phase windows. The remaining visits can be arbitrarilty placed within the entire 0.9515-0.9580 phase window. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9515-0.9580 phase range. 1422469714000 73.5154648402328 (Tic-Visit :proposal-id 13665 :visit-id "26" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:03:12.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1445120 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "26" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "26" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "26" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "26" :orbit-number 4 :pcs-time 222 :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 2992 :pcs-gap 0 ) false 4 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. First (of two) STIS/G750L transit of GJ 436b. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-436 STIS visit observes GJ-436 during the transit of GJ-436b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9410-0.9455 in planet orbital phase, corresponding to a 17 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three WFC3 visits, the first visit has been scheduled to begin within the first 8.5 minutes of the phase windows and the second visit has been scheduled to begin in the last 8.5 min of the phase windows. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9410-0.9455 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). We also include orientation restrictions intended to avoid overlapping spectra with a H=13.1 star located at a distance of 64" (6"S, 63"W) from GJ 436 (H=6.3). We find that we should avoid rotation angles between -10 to +20 degrees and 170 to 200 degrees in order to preserve a minimum separation of 12" in the Y (vertical) direction between the two spectra. We use 2MASS J2000 coordinates for both objects, and take into account GJ 436b's high proper motion of [896.1, -813.5] mas/yr to calculate the J2012 coordinates and corresponding rotation angle constraints. 1433905115000 113.9138886134674 (Tic-Visit :proposal-id 13665 :visit-id "27" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:03:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 436064 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "27" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2643 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "27" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2756 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "27" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2756 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "27" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2756 :al-overhead-at-end 120 :internal-dur-at-end 666 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. Second (of two) STIS/G750L transit of GJ 436b. It is essential for the four orbits in each visit to be scheduled in a contiguous block. These orbits should be free of the SAA. Orbits 3 in each GJ-436 STIS visit observes GJ-436 during the transit of GJ-436b. To maximize the time of in-transit observation, the total allowed window for the start of the first exposure in orbit 1 is 0.9410-0.9455 in planet orbital phase, corresponding to a 17 minute interval. In order to also ensure complete coverage of the transit light curve when combining the three WFC3 visits, the first visit has been scheduled to begin within the first 8.5 minutes of the phase windows and the second visit has been scheduled to begin in the last 8.5 min of the phase windows. If the first or second visits place a significant barrier to scheduling, the requirements for all visits and may be relaxed to 0.9410-0.9455 phase range. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). We also include orientation restrictions intended to avoid overlapping spectra with a H=13.1 star located at a distance of 64" (6"S, 63"W) from GJ 436 (H=6.3). We find that we should avoid rotation angles between -10 to +20 degrees and 170 to 200 degrees in order to preserve a minimum separation of 12" in the Y (vertical) direction between the two spectra. We use 2MASS J2000 coordinates for both objects, and take into account GJ 436b's high proper motion of [896.1, -813.5] mas/yr to calculate the J2012 coordinates and corresponding rotation angle constraints. (Tic-Visit :proposal-id 13665 :visit-id "28" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:03:26.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 436064 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "28" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2643 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "28" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2756 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "28" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2756 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "28" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2756 :al-overhead-at-end 120 :internal-dur-at-end 666 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2993 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. WFC3/G141 transit visits of EPIC2019_WFC3_1. It is essential for the orbits in each visit to be scheduled in a contiguous block. 1449405547000 293.7345031221558 (Tic-Visit :proposal-id 13665 :visit-id "29" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:03:57.0" :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 13665 :visit-id "29" :obset-id "29" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "29" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "29" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "29" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "29" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "29" :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 2992 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. WFC3/G141 transit visits of EPIC2019_WFC3_1. It is essential for the orbits in each visit to be scheduled in a contiguous block. (Tic-Visit :proposal-id 13665 :visit-id "30" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:04:29.0" :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 13665 :visit-id "30" :obset-id "30" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "30" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "30" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "30" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "30" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "30" :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 2992 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. WFC3/G141 transit visits of EPIC2019_WFC3_1. It is essential for the orbits in each visit to be scheduled in a contiguous block. 1457941093000 160.088494298986 (Tic-Visit :proposal-id 13665 :visit-id "35" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:05:02.0" :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 13665 :visit-id "35" :obset-id "35" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "35" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "35" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "35" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "35" :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "35" :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 2992 :pcs-gap 0 ) false 5 0 The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. It is essential for the four orbits in each visit to be scheduled in a contiguous block. We disable auto-wavecals, which improves our observing efficiency and repeatability. We opt for only a single GO-wavecal (at the end of each visit) because the GO-wavecal requires a different aperture (52x0.2 instead of the 52x2 used for science observations). To minimize disruption to the observatory, we therefore defer the GO wavecal until the end of each visit. This strategy has been successfully employed in past programs, e.g. 12473 (PI Sing). 1446614576000 116.68419061493648 (Tic-Visit :proposal-id 13665 :visit-id "34" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:05:12.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 702576 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "34" :obset-id "34" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "34" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2626 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "34" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "34" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "34" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2758 :al-overhead-at-end 123 :internal-dur-at-end 417 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3017 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. It is essential for the four orbits in each visit to be scheduled in a contiguous block. 1458651689000 343.72607637515193 (Tic-Visit :proposal-id 13665 :visit-id "36" :proposal-version -1 :trans-version "20160129" :date "21-Feb-2016 21:05:35.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 702576 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "36" :obset-id "36" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "36" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2626 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "36" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "36" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "36" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2758 :al-overhead-at-end 123 :internal-dur-at-end 417 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3017 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. It is essential for the four orbits in each visit to be scheduled in a contiguous block. (Tic-Visit :proposal-id 13665 :visit-id "37" :proposal-version -1 :trans-version "20160129" :date "07-Apr-2016 19:29:42.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 702576 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "37" :obset-id "37" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "37" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2626 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "37" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "37" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "37" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2758 :al-overhead-at-end 123 :internal-dur-at-end 417 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3017 :pcs-gap 0 ) false 4 0 Explicit WAVECAL, auto-waves disabled The scheduling data was generated by CASM 24.0. CASM was run in Phase II mode. It is essential for the four orbits in each visit to be scheduled in a contiguous block. (Tic-Visit :proposal-id 13665 :visit-id "38" :proposal-version -1 :trans-version "20160129" :date "07-Apr-2016 19:32:10.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 5 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 883408 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13665 :visit-id "38" :obset-id "38" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13665 :visit-id "38" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2626 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "38" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "38" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "38" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2758 :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 3017 :pcs-gap 0 ) (Tic-Orbit :proposal-id 13665 :visit-id "38" :orbit-number 5 :pcs-time 222 :si-vis-utilization 2758 :al-overhead-at-end 123 :internal-dur-at-end 429 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3017 :pcs-gap 0 ) false 5 0 Explicit WAVECAL, auto-waves disabled