This proposal is for pure parallel orbits. Two demonstrative observations around the intended targets were included for the proposal (summing to 2 orbits). If additional detail is required, please contact the PI! 2066910367 Assigned ID: 772 ----- Attempting Submission 1 (Fri Apr 05 21:13:18 GMT 2019) ----- HST Phase I Proposal 772 (Cyc27_IR_TRGB_Calib_1pmFriday.pdf.apt) successfully submitted. Receipt: # 772-1 ----- Attempting Submission 2 (Fri Apr 05 22:46:54 GMT 2019) ----- HST Phase I Proposal 772 (Cyc27_IR_TRGB_Calib_1pmFriday.pdf.apt) successfully submitted. Receipt: # 772-2 ----- Attempting Submission 3 (Fri Apr 05 22:51:21 GMT 2019) ----- ----- Attempting Submission 4 (Sun Apr 07 03:38:32 GMT 2019) ----- The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity The number of Visits in an observation may not exceed the limit derived from the selected opportunity Illegal selection: 16109_07 [RA: 165.46627275594 Dec: -34.70473131948 ] 1 orbit: [1707]. Illegal selection: 16109_08 [RA: 165.46627275594 Dec: -34.70473131948 ] 1 orbit: [1707]. Illegal selection: 16109_09 [RA: 165.46627275594 Dec: -34.70473131948 ] 1 orbit: [1707]. Illegal selection: 16109_10 [RA: 165.46627275594 Dec: -34.70473131948 ] 1 orbit: [1707]. Illegal selection: 16109_11 [RA: 165.46627275594 Dec: -34.70473131948 ] 1 orbit: [1707]. Illegal selection: 16109_12 [RA: 165.46627275594 Dec: -34.70473131948 ] 1 orbit: [1707]. Added opportunity 16366_4S. -762420399 ----- Attempting Submission 1 (Fri May 08 19:00:40 GMT 2020) ----- ----- Attempting Submission 2 (Wed May 20 15:34:09 GMT 2020) ----- ----- Attempting Submission 3 (Mon Sep 21 15:40:22 GMT 2020) ----- HST Phase II Proposal 16358 successfully submitted. Receipt: # 16358-3 ----- Attempting Submission 4 (Mon Sep 21 15:54:51 GMT 2020) ----- ----- Attempting Submission 5 (Tue Nov 03 01:09:10 GMT 2020) ----- Your proposal could not be saved. Submission aborted. ----- Attempting Submission 6 (Thu Nov 12 05:42:15 GMT 2020) ----- ----- Attempting Submission 7 (Sat Dec 26 17:42:19 GMT 2020) ----- Your proposal could not be saved. Submission aborted. ----- Attempting Submission 8 (Mon Mar 29 14:47:24 GMT 2021) ----- ----- Attempting Submission 9 (Fri Apr 23 16:24:50 GMT 2021) ----- ----- Attempting Submission 10 (Wed May 19 00:34:12 GMT 2021) ----- ----- Attempting Submission 11 (Sun Nov 14 18:25:47 GMT 2021) ----- ----- Attempting Submission 12 (Wed Feb 09 19:37:07 GMT 2022) ----- ----- Attempting Submission 13 (Tue Apr 12 21:02:50 GMT 2022) ----- Withdrawn visits Securing the Absolute Scale for the IR-TRGB Distance Ladder The tension in the value of the Hubble constant as derived from the distance scale in the local universe and modeled from the anisotropies in the Cosmic Microwave Background continues to grow. While theoretical reasons for the tension are being explored, determining if systematics within rungs of the distance scale is the cause of the tension requires the use of independent techniques. Of late the tip of the red giant branch (TRGB) has provided a key test of the calibration of type supernova Ia by Cepheids and has not yet revealed a systematic effect at this stage. Another concern is both expanding the Supernova Ia calibration sample, itself, and expanding the sample beyond star-forming hosts due to variance in the supernova with host properties. The TRGB applied in the infrared is poised to be a powerful tool to probe ever larger volumes and reach a wider set of supernova Ia hosts. However, anchoring the IR-TRGB is challenging because the two primary systems, the Milky Way and the Large Magellanic Cloud, only have observations in the 2MASS filter system. Comparison of IR-TRGB calibrations from the ground suggests that there are strong differences between the WFC3/IR and 2MASS filter system that are hard to reconcile at distance-ladder required precision. Here pure parallel orbits in Large and Small Magellanic Cloud are proposed to produce a robust filter-calibration to secure the foundation for the IR-TRGB distance scale. The proposal uses a combination of IR imaging and spectroscopy to enable a broader set of calibrations for other facilities where the IR-TRGB can be applied. This proposal observes with WFC3/IR in pure parallel mode. It will attempt to obtain 3-band photometry using the shortest exposures possible and 2-grisms for a set of fields in the LMC and SMC. The observations will have multiple reads to help with random errors and multi-visit fields will be used to constrain systematic errors. The specifications of MULTIACCUM are set to keep the targets from saturating and, if possible, minimize the systematics due to persistence and non-linearity. This team combines scientific and technical experience from the Carnegie-Chicago Hubble Program (CCHP, PI: Freedman; Madore, Rich, Seibert, Beaton, Hoyt, Neeley, Monson), the ACS Nearby Galaxies (ANGST) and related programs (PI: Dalcanton; Durbin), and ground-based efforts in the Large Magellanic Cloud (Nidever, Beaton) to adequately cover the range of expertise required for this program. First, the CCHP has been producing high-precision distances using the tip of the red giant branch in the optical and begun branching into the first precision application of the technique in the infrared (Madore, Hoyt, Freedman, Beaton). A pipeline has been constructed that fully reduces raw frames and produces systematics-controlled photometry for objects over a range of 16 magnitudes in distance modulus (Beaton, Seibert, Hoyt). The pipeline is being expanded to contain a module for WFC3/IR using data obtained in the CCHP program (Beaton, Seibert, Neeley). The CCHP obtained direct observations with WFC3/IR of bright RR Lyrae stars obtained in special observing modes and requiring special analyses (Rich, Beaton, Seibert). Second, the ACS Nearby Galaxies programs have accumulated extensive multi-instrument HST observations for dozens of objects in the nearby universe (Dalcanton, Durbin). Currently, the WFC3/IR data is being systematically reprocessed in combination with higher spatial resolution ACS observations with the goal of better constraining the IR-TRGB in these more distant objects via an archival proposal (PI Durbin). Durbin worked at STScI as a post-bac and has extensive technical expertise with WFC3/IR. Third, our spectroscopic experience stems from numerous on-going projects probing the Galaxy and its neighbors in the Local Group. Noteworthy experience in the NIR at medium resolution via the Sloan Digital Sky Survey III sub-survey APOGEE2, which contains an expansive program covering the Magellanic Clouds (Nidever, Beaton). Team members have access to facilities in the southern hemisphere to obtain complementary data if required (either higher precision photometry or stellar characteristics from spectroscopy) using Las Campanas Observatory (Beaton, Rich, Madore, Seibert), existing survey data from the Sloan Digital Sky Survey (Beaton, Nidever) or the Magellanic Periphery Surveys with the Dark Energy Survey Camera (Nidever). Lastly, members of the team are constructing a small aperture (17-inch), robotic, infrared telescope for operation at Las Campanas Observatory (Beaton, Monson, Madore) for which the primary program will be the acquisition of precise magnitudes for TRGB stars in the Galaxy and in the Magellanic Clouds in the 2MASS system in complement to these observations. 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The F110W (wJ_img) is the most likely to be saturated and thus it comes last. 1632399246000 279.1616070731175 (Tic-Visit :proposal-id 16358 :visit-id "39" :proposal-version -1 :trans-version "20211222" :date "12-Apr-2022 13:10:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 626720 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16358 :visit-id "39" :obset-id "39" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16358 :visit-id "39" :orbit-number 1 :pcs-time 0 :si-vis-utilization 456 :al-overhead-at-end 0 :internal-dur-at-end 2245 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2252.0 :pcs-gap 0 ) true 1 0 1972.0 /private/var/folders/72/z00tr7ks3b5gmx_24dfmqmz40000gn/T/OPVisit11041308592820770997.xml This orbit is broken into 5 exposures that sum up to 30 full frame reads. 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F153M this time is SPARS5 with 3 reads, and F110W has been reduced to 4 reads. 1623129308000 173.6833323810598 (Tic-Visit :proposal-id 16358 :visit-id "32" :proposal-version -1 :trans-version "20211222" :date "12-Apr-2022 13:10:06.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 626720 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16358 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16358 :visit-id "32" :orbit-number 1 :pcs-time 0 :si-vis-utilization 454 :al-overhead-at-end 0 :internal-dur-at-end 2187 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 1972.0 :pcs-gap 0 ) true 1 0 2261.0 /private/var/folders/72/z00tr7ks3b5gmx_24dfmqmz40000gn/T/OPVisit17656077985316487726.xml This orbit is broken into 5 exposures that sum up to 30 full frame reads. 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F153M this time is SPARS5 with 3 reads, and F110W has been reduced to 4 reads. 1627983765000 285.7361658512483 (Tic-Visit :proposal-id 16358 :visit-id "40" :proposal-version -1 :trans-version "20211222" :date "12-Apr-2022 13:10:06.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 626720 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16358 :visit-id "40" :obset-id "40" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16358 :visit-id "40" :orbit-number 1 :pcs-time 0 :si-vis-utilization 454 :al-overhead-at-end 0 :internal-dur-at-end 2309 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2261.0 :pcs-gap 0 ) true 1 0 2097.0 /private/var/folders/72/z00tr7ks3b5gmx_24dfmqmz40000gn/T/OPVisit7869560450259347140.xml This orbit is broken into 6 exposures that sum up to 30 full frame reads. This means that the buffer can hold the data until the end and dump onces the primary is complete. The F110W (wJ_img) is the most likely to be saturated and thus it comes last. 1647824483000 166.30929858527912 (Tic-Visit :proposal-id 16358 :visit-id "34" :proposal-version -1 :trans-version "20211222" :date "12-Apr-2022 13:10:07.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 626720 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16358 :visit-id "34" :obset-id "34" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16358 :visit-id "34" :orbit-number 1 :pcs-time 0 :si-vis-utilization 456 :al-overhead-at-end 0 :internal-dur-at-end 2373 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2097.0 :pcs-gap 0 ) true 1 0 2537.0 /private/var/folders/72/z00tr7ks3b5gmx_24dfmqmz40000gn/T/OPVisit414531464909064776.xml This orbit is broken into 6 exposures that sum up to 30 full frame reads. 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This means that the buffer can hold the data until the end and dump onces the primary is complete. The F110W (wJ_img) is the most likely to be saturated and thus it comes last. 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The F110W (wJ_img) is the most likely to be saturated and thus it comes last. The timing of the H and J img+grism is flipped in the 2nd visit to test for sub-orbit systematics. Additionally, this orbit tests the F153M exposure configuration of 2 reads with SPARS10 instead of 3 with SPARS5, with the additional read returned to the F160W exposure. 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