Submission 31499459711Assigned ID: 3143
----- Attempting Submission 1 (Fri Mar 25 05:29:39 GMT 2022) -----
HST Phase I Proposal 3143 successfully submitted.
Receipt: # 3143-1
----- Attempting Submission 2 (Fri Mar 25 18:45:33 GMT 2022) -----
HST Phase I Proposal 3143 successfully submitted.
Receipt: # 3143-2
----- Attempting Submission 3 (Fri Mar 25 19:00:34 GMT 2022) -----Third submission, subsequent to HOPR 92582 for HST program 17154.
Visit 3A is a clone of 2A, and *urgent* scheduling is requested (prior to 26 July)
to keep this observation contemporaneous with visits 2A-2F as a transient-search.
Minor changes from 2A to 3A:
* ORI changed, for compatibility through 25 July;
* targeting slid very slightly, to avoid high-value JWST transients falling into ACS chip gap;
* exposures lengthened to obtain more CTE-mitigating sky background --- no impact to schedulability pre-26-July
If guidestar check fails, and/or scheduling is impossible prior to 26 July --- when visibility window closes --- visit 3A will be further amended.1749134414----- Attempting Submission 1 (Tue Jul 12 21:56:22 GMT 2022) -----
----- Attempting Submission 2 (Wed Jul 13 13:13:43 GMT 2022) -----
----- Attempting Submission 3 (Tue Jul 18 20:20:28 GMT 2023) -----Third submission, subsequent to HOPR 92582 for HST program 17154.
Visit 3A is a clone of 2A, and *urgent* scheduling is requested (prior to 26 July)
to keep this observation contemporaneous with visits 2A-2F as a transient-search.
Minor changes from 2A to 3A:
* ORI changed, for compatibility through 25 July;
* targeting slid very slightly, to avoid high-value JWST transients falling into ACS chip gap;
* exposures lengthened to obtain more CTE-mitigating sky background --- no impact to schedulability pre-26-July
If guidestar check fails, and/or scheduling is impossible prior to 26 July --- when visibility window closes --- visit 3A will be further amended.ACS Observations in a JWST CVZ Field --- providing the missing link for a JWST time-domain science initiativeWe propose ACS F435W, F606W, and F814W imaging in the IRAC Dark Field (IDF), which is in the JWST continuous viewing zone (CVZ) and will be observed by JWST GTO program #2738 in three epochs in Cycle 1 using NIRCam. The 3-epoch JWST data (>28.5 mag) will enable time-domain science such as finding and studying core-collapse supernovae in dusty starbursts and high-z Type Ia supernovae potentially to z=6. Reaching the full scientific potential, however, requires high-resolution data in the optical bands that are either not accessible to or not optimized with JWST. Our program will take advantage of the overlap in mission life of HST and JWST to fill in this crucial gap. To maximize the return, the proposed ACS observations will be split into two epochs that are near-contemporaneous with the 2nd and 3rd epochs of the JWST GTO observations, respectively. (The JWST schedule will be announced in April 2022.) The contemporaneous ACS observations will enable a joint analysis of the time-domain events found in the NIRCam data. The complementary ACS data will be critical because any time-dependent evolution should be removed from the SEDs for a proper analysis. With these data, we will be able to: 1) identify and study the exact sites (within the host galaxies) associated with the events; 2) estimate the dust extinction corrections appropriate for the events; and 3) constrain the source redshifts when the association with the host galaxy is unclear or when the host galaxy is too faint for spectroscopy. In addition, the combined, "static" ACS images will enable a slew of extragalactic studies that require a broad wavelength sampling from optical to near-IR (e.g., z>10 dropout searches).We propose ACS F435W, F606W, and F814W imaging in the IRAC Dark Field (IDF), which is in the JWST continuous viewing zone (CVZ) and will be observed by JWST GTO program #2738 in three epochs in Cycle 1 using NIRCam. The 3-epoch JWST data (>28.5 mag) will enable time-domain science such as finding and studying core-collapse supernovae in dusty starbursts and high-z Type Ia supernovae potentially to z=6. Reaching the full scientific potential, however, requires high-resolution data in the optical bands that are either not accessible to or not optimized with JWST. Our program will take advantage of the overlap in mission life of HST and JWST to fill in this crucial gap. To maximize the return, the proposed ACS observations will be split into two epochs that are near-contemporaneous with the 2nd and 3rd epochs of the JWST GTO observations, respectively. (The JWST schedule will be announced in April 2022.) The contemporaneous ACS observations will enable a joint analysis of the time-domain events found in the NIRCam data. The complementary ACS data will be critical because any time-dependent evolution should be removed from the SEDs for a proper analysis. With these data, we will be able to: 1) identify and study the exact sites (within the host galaxies) associated with the events; 2) estimate the dust extinction corrections appropriate for the events; and 3) constrain the source redshifts when the association with the host galaxy is unclear or when the host galaxy is too faint for spectroscopy. In addition, the combined, "static" ACS images will enable a slew of extragalactic studies that require a broad wavelength sampling from optical to near-IR (e.g., z>10 dropout searches).Our team members have extensive experience that will ensure this program's success. Seven of us have led at least one past HST program. All members are experts in the study of star formation and/or AGN at high redshifts, and have their expertise at different wavelength regimes. We highlight the following aspects of the team expertise that are the most relevant to the execution of this program.
-- HST Observational Design: Dr. Norman Grogin, Dr. Rolf Jansen
-- HST Data Reduction: Dr. Anton Koekemoer, Dr. Rolf Jansen, Prof. Haojing Yan, Dr. Seth Cohen, Dr. Zhiyuan Ma
-- Time-domain Science: Prof. Lifan Wang, Prof. Haojing Yan, Prof. John Beacom, Dr. Norman Grogin, Dr. Anton Koekemoer
-- Supernova-specific Science: Prof. Lifan Wang
-- FIR/Submm Science: Prof. Min Yun, Prof. Haojing Yan, Dr. Zhiyuan Ma, Dr. Jiasheng Huang, Dr. Cheng Cheng, Dr. Giovanni Fazio, Dr. Steven Willner
-- Morphological Studies: Prof. Christopher Conselice, Prof. Haojing Yan, Dr. Cheng Cheng
-- Galaxy formation at high-z: Prof. Haojing Yan, Prof. Rogier Windhorst, Dr. Seth Cohen, Dr. Jiasheng Huang
We note all co-I's of this program are team members of the JWST Interdisciplinary Scientist GTO Program #1176 (PI Windhorst), which this proposed ACS program will complement.Galaxies6falsefalsefalsefalsefalsefalsefalsefalseSUPPORTEDUNIDENTIFIEDHIGH LATITUDE FIELDJ2000J2000UNIDENTIFIEDHIGH LATITUDE FIELDJ2000J2000UNIDENTIFIEDHIGH LATITUDE FIELDJ2000J2000ACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF606WACS/WFCImagingNoNoF814WACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF606WACS/WFCImagingNoNoF814WACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF606WACS/WFCImagingNoNoF814WACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF606WACS/WFCImagingNoNoF814WHst Same orient constraint links visits (1A 1B 1C 1D 1E 1F)The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.1672459035000332.0(Tic-Visit
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