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Assigned ID: 3207
----- Attempting Submission 1 (Fri Mar 25 12:27:48 GMT 2022) -----
HST Phase I Proposal 3207 successfully submitted.
Receipt: # 3207-1
----- Attempting Submission 2 (Fri Mar 25 13:19:52 GMT 2022) -----
The number of orbits used exceeds the number allocated
SAME POS MAY NOT BE APPROPRIATE
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SAME POS MAY NOT BE APPROPRIATE
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SAME POS MAY NOT BE APPROPRIATE
SAME POS MAY NOT BE APPROPRIATE
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SAME POS MAY NOT BE APPROPRIATE
SAME POS MAY NOT BE APPROPRIATE
SAME POS MAY NOT BE APPROPRIATE
SAME POS MAY NOT BE APPROPRIATE
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ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
ORBITAL VISIBILITY OVERRUN
created visits 55, 57, 58 which replace the orbits 5, 7, and 8 with problems due to guiding failures
-363015778
----- Attempting Submission 1 (Wed Jul 13 14:57:11 GMT 2022) -----
HST Phase II Proposal 17172 successfully submitted.
Receipt: # 17172-1
----- Attempting Submission 2 (Mon Oct 24 08:07:18 GMT 2022) -----
HST Phase II Proposal 17172 successfully submitted.
Receipt: # 17172-2
----- Attempting Submission 3 (Tue Oct 25 19:31:10 GMT 2022) -----
HST Phase II Proposal 17172 successfully submitted.
Receipt: # 17172-3
----- Attempting Submission 4 (Wed Oct 26 05:55:49 GMT 2022) -----
HST Phase II Proposal 17172 successfully submitted.
Receipt: # 17172-4
----- Attempting Submission 5 (Wed Oct 26 21:52:03 GMT 2022) -----
HST Phase II Proposal 17172 successfully submitted.
Receipt: # 17172-5
----- Attempting Submission 6 (Mon Oct 31 21:21:54 GMT 2022) -----
----- Attempting Submission 7 (Tue Apr 23 17:15:09 GMT 2024) -----
Grism exposures are set to be 'same pos targ' as the F140W exposure before them. There is a pos targ offset in each F140W exposure.
This was the same warning as with the original submission and ensures the orbits are at the correct orients.
Caught in the act: Galaxy quenching beyond the core of a redshift two galaxy cluster?
Cluster environments in the local universe are dominated by passive, quiescent galaxies while proto-clusters at z>2 typically contain large fractions of actively star-forming galaxies. The physics underlying this observed transformation of the cluster member population has been a long standing puzzle in astronomy. The cluster quenching efficiency appears to rapidly increase over cosmic time but whether this is due to the pre-processing of galaxies in group environments prior to infall or occurs during accretion into the cluster itself is unknown. Our understanding has been limited by the lack of virialized clusters discovered at the critical transformational redshift of z~2, until now.
We propose HST observations of XLSSC 122 - the highest redshift (z=1.98), virialized, massive galaxy cluster. We will utilize G141 grism observations to determine the redshifts of galaxies out to twice the cluster virial radius and combine these with WFC3 F140W/F105W and ACS F814W imaging to constrain the star-formation activity in these galaxies. These data will provide unique, unparalleled insight into the cosmic evolution of environmental quenching and unveil its impact in the cluster outskirts and in nearby groups and filaments.
The observations are arranged in vists which reflect both the orbit and orient.
We have chosen to have a visit represent a consistent orient and pointing.
This means we have 8 visits where the grism+direct filters is used as prime each of 2 orbits in length.
~52 min visibility 1 orbit = ~3120 sec so 2 orbits ~6240 sec
ABBA stratergy
A = F140W ~200s
B = G141 ~ 1300s
Total F140W ~1600s per Pointing
Total G141 ~10400s per Pointing
Prime: Grism+F140W
Parallel: ACS F814W
V1 - Pointing 1, orient 1, 2 orbits
V2 - Pointing 1, orient 2, 2 orbits
V3 - Pointing 2, orient 3, 2 orbits
V4 - Pointing 2, orient 4, 2 orbits
V5 - Pointing 3, orient 5, 2 orbits
V6 - Pointing 3, orient 6, 2 orbits
V7 - Pointing 4, orient 7, 2 orbits
V8 - Pointing 4, orient 8, 2 orbits
We have 4 visits where F105W is used as prime each of 1 orbit in length.
~52 min visibility 1 orbit = ~3120 sec
Prime: F105W
Parallel: ACS F814W
V9 - Pointing 1, orient 1, 1 orbits
V10 - Pointing 2, orient 2, 1 orbits
V11 - Pointing 3, orient 3, 1 orbits
V12 - Pointing 4, orient 4, 1 orbits
We have 4 visits where F140W is used as prime each of 1 orbit in length.
~52 min visibility 1 orbit = ~3120 sec
Prime: F140W
Parallel: ACS F814W
V13 - Pointing 1, orient 5, 1 orbits
V14 - Pointing 2, orient 6, 1 orbits
V15 - Pointing 3, orient 7, 1 orbits
V16 - Pointing 4, orient 8, 1 orbits
We have 4 visits where F814W is used as prime each of 2 orbit in length.
~52 min visibility so 2 orbit = ~6240 sec
Prime: ACS F814W
Parallel: G141+F140W
V17 - Pointing 1, orient 9, 2 orbits
V18 - Pointing 2, orient 9, 2 orbits
V19 - Pointing 3, orient 10, 2 orbits
V20 - Pointing 4, orient 10, 2 orbits
Orients
Orients have constraint so that grisms are offset for contamination and parallels are distribtued.
Pointings
Offsets from center of old observations:
Center: 02 17 44.1900, -03 45 31.46
Offsets were determined from ds9. These offsets are modified by a couple of arseconds for the F814W exposures to ensure they do not leave a gap where the BCG is and BCG is not too close to chip edge.
Pointing 1 - SE - 60 arcsec S, ~90 arcsec E, 02 17 50.8452 , -03 46 35.21
Pointing 2 - NE - 60 arcsec N, ~90 arcsec E, 2:17:50.8449, -3:44:35.680
Pointing 3 - NW - 60 arcsec N, ~90 arcsec W, 2:17:38.2667, -3:44:35.680
Pointing 4 - SW - 60 arcsec S, ~90 arcsec W, 2:17:38.2665, -3:46:35.209
Dr. Willis has expertise in HST WFC3 imaging and grism observations of distant galaxy clusters and their application to determining the physical properties of member galaxies. Ms Leste is Dr. Willis' MSc student.
Dr. Canning has expertise in HST data reduction including WFC3 grism data and their application to galaxy and AGN evolution in distant cluster environments. Ms. Alfarsy is a graduate student working with Dr. Canning.
Drs. Allen and Mantz are experts in galaxy clusters and the estimation of phsyical properties such as mass, radius, centroid and morphology from both X-ray and SZ data sets.
Dr. Brammer is an expert on many aspects of HST WFC3 instrument operation and data reduction including Grism observations and is an expert in galaxy evolution studies.
Dr. Stanford is an expert in infrared studies of high redshift galaxy clusters.
Dr. Burchett has expertise in multi-wavelength studies of galaxy evolution including Lyman-break galaxies and Lyman-alpha imaging.
Galaxies
Large Scale Structure of the Universe
6
false
false
false
false
false
false
false
false
SUPPORTED
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
RICH CLUSTER
J2000
J2000
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F140W
WFC3/IR
Imaging
No
No
F105W
WFC3/IR
Imaging
No
No
F105W
WFC3/IR
Imaging
No
No
F140W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F814W
WFC3/IR
Imaging
No
No
F140W
WFC3/IR
Imaging
No
No
F105W
POS-TARG
DITHER
DITHER
4
5.183
WFC3-IR-DITHER-BOX-MIN
false
74.653
true
0.365
0.572
2
41.859
POS-TARG
WFC3-IR-DITHER-BLOB
18.528
1
false
The scheduling data was generated by CASM 30.3.
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