0
Assigned ID: 742
----- Attempting Submission 1 (Fri Apr 10 20:05:00 GMT 2015) -----
Dear PC, this is the 2nd submission of the phase II proposal for our program GO-14182 (Coma Cluster Core Project).
Compare to the 1st phase II submission, the following changes were applied:
- Unlink visits 02-14 and 18 from visit 01 (since all these visits will not schedule at the same ORIENT as visit 01)
ok
- Visit 01 will schedule at ORIENT range 310-330 deg using single guide star
or schedule at ORIENT range 290-300 using guide star pairs
go for ORIENT range 310-330
- Visit 02 will schedule at ORIENT range 310-330 deg using single guide star
ok
- Visit 04 will schedule at ORIENT range 240-260 deg using single guide star
ok, but would a range 220-240 also work? If yes, please use that. And move visit4 slightly to the north:
Move: 4 TILE-04
From: <13:00:0.8629 +27:55:45.53>
To: <13:00:00.85403 +27:55:55.5974>
This is to preserve field integrity of the survey footprint.
- Visit 10 will schedule at ORIENT range 300-310 deg using single guide star
ok
- Visit 18 will schedule at ORIENT range 240-260 deg using single guide star
Would a range 220-240 work as well? If yes, please use that, and move visit 18 like
Move: 18 TILE-18
From: <12:59:31.6195 +28:01:30.16>
To: <12:59:31.61372 +28:01:36.2004>
This is to preserve maximum object coverage in this region.
- Visits 03, 05-09, and 11-14 will schedule at ORIENT range 310-330 deg using guide star pairs so the "SAME ORIENT AS" requirement will need to be removed and the ORIENT range 310-330 deg added
ok
No changes are needed for visits 15-17 and 19-21 as they schedule fine.
ok
Kind regards,
Thomas Puzia & team
409386177
----- Attempting Submission 1 (Tue Jul 21 15:55:38 GMT 2015) -----
HST Phase II Proposal 14182 (Coma_c23_ph2_v1.apt) successfully submitted.
Receipt: # 14182-1
----- Attempting Submission 2 (Thu Oct 01 20:23:41 GMT 2015) -----
0
The Coma Cluster Core Project
We propose to use WFC3 to perform a contiguous, high spatial resolution UV (F336W) and IR (F160W) survey of an area of ~100 square arcminutes in the core of the Coma cluster of galaxies. The area is already surveyed by our group in optical passbands with the ACS F475W and F814W filters. The new UV and IR data will be used, in combination with existing ACS data, for studies of the populations of Globular Clusters (GCs), Ultra-Compact Dwarf Galaxies (UCDs), and Nuclear Star Clusters (NSCs) in Coma galaxies and in the cluster environment. Using an innovative technique developed by members of our team, we can essentially eliminate foreground and background contamination from samples of compact stellar systems. This allows us, for the first time, to perform the most detailed assessment and study of the very large population of Intracluster GCs in a nearby rich cluster (i.e. Coma), to find why this population is so abundant, and why it contains such a significant metal-rich component, which is unexpected if the origin is from stripping of clusters from low-mass dwarf galaxies. For NSCs, the additional passbands will allow us to test predictions of the relationship between NSC properties and age and metallicity gradients in the host galaxies, which in turn helps to understand the NSC formation mechanisms, and the timescale and feedback process that truncate the star formation. This is the last opportunity to perform a rest-frame UV survey at z=0, given the rapidly declining capability of WFC3/UVIS and the fact that there is no prospect for a future UV space mission for decades to come.
We target the core region of the Coma galaxy cluster. The observations are arranged in a mosaic of 21 pointings (as illustrated in Figure 2 of the phase I proposal, with corresponding tile numbers increasing E->W and S->N, starting with the SE corner). The observation for each tile are completed in one visit, which consits of three primary orbits and coordinated parallel observations. To optimize the footprint of the parallel observations we request the HST roll angle to be constrained to place ACS/WFC and WFC3 along the optimal orientation of 320 degrees for the two southernmost rows of mosaic tiles (1-14 and 18), and 140 degrees for the remaining tiles (15-17 and 19-21), both constraints having a tolerance within +/-10 degrees. However, once a roll angle is set for each of the two subsets, all tiles in each subset shall be observed with the same roll angle in order to preserve field coherence and data homogeneity. This will also guarantee that the survey footprint of archival ACS data is expanded by ~65%.
The primary observations are conducted with WFC3/UVIS+F336W (2 orbits) and WFC3/IR+F160W (1 orbit). Coordinated observations are taken with ACS/WFC+F475W in parallalel with WFC3/UVIS, and with ACS/WFC+F814W in parallel with the WFC3/IR frames. At least two dithered positions are used for each filter to allow a robust elimination of hot pixels and cosmic ray hits during the analysis. The F336W observations include one short exposure at the beginning of each orbit to avoid source saturation. Within the buffer dump constraints of the primary observations we obtain three sub-exposures per orbit in F475W and three long and one shorter exposure in F814W with ACS.
UNRESOLVED STELLAR POPULATIONS AND GALAXY STRUCTURE
12
false
false
false
false
false
false
SUPPORTED
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy NGC4906 is V=14.08 mag. Brightest star in FOV has B=15.06, V=14.4, H=12.71 (2MASS J13003781+2755236).
J2000
J2000
B=15.2 H=11.576
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy SDSS J130024.82+275535.8 is V=17.3 mag. Brightest star in FOV has B=16.66, V=15.7, H=13.49 (2MASS J13002799+2754384).
J2000
J2000
B=16.66 H=13.49
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy 2MASX J13001877+2756135 is B=15.8 mag. Brightest star in FOV has B=12.55, V=12.32, H=11.19 (TYC 1995-1988-1).
J2000
J2000
B=12.55 H=11.19
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy 2MASX J12595670+2755483 is V=15.4 mag. Brightest star in FOV has B=14.45, V=13.76, H=11.28 (2MASS J13000364+2755351).
J2000
J2000
B=14.45 H=11.28
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy NGC4876 is V=14.2 mag. Brightest star in FOV has B=16.21, V=15.39, H=13.29 ([EDG2007] 99).
J2000
J2000
B=16.21 H=13.29
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy NGC4875 is V=14.8 mag. Brightest star in FOV has u=17.6, g=17.4, z=17.8 (WD: A2 287).
J2000
J2000
B=15.9 H=11.8
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy NGC4869 is V=13.2 mag. Brightest star in FOV has B=13.65, V=12.1, H=10.23 (TYC 1995-1839-1).
J2000
J2000
B=13.65 H=10.23
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy 2MASX J13004285+2757476 is V=15.0 mag. Brightest star in FOV has B=15.69, V=14.47, H=11.46 (2MASS J13004077+2757131).
J2000
J2000
B=15.69 H=11.46
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC4033 is V=15.23 mag. Brightest star in FOV has B=16.58, V=15.66, H=13.73 (2MASS J13002195+2757230).
J2000
J2000
B=16.58 H=13.73
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy NGC4889 is V=11.3 mag. Brightest star in FOV has B=15.0, V=14.02, H=11.17 (2MASS J13001074+2757516).
J2000
J2000
B=13.0 H=8.7
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy NGC4886 is V=14.3 mag. NGC4889 straddles the eastern edge of the tile. Brightest star in FOV (southern edge) has B=18.98, V=18.24, H=17.09 (2MASS J12595810+2757149).
J2000
J2000
B=15.1 H=11.4
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC3998 is V=14.6 mag. Brightest star in FOV has B=18.54, V=17.28, H=13.8 (2MASS J12595201+2757405).
J2000
J2000
B=15.9 H=11.9
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy NGC4874 is V=11.4 mag. Brightest star in FOV has B=22.08, V=19.76, H=13.95 (2MASS J12593660+2759042).
J2000
J2000
B=13.7 H=9.0
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC3968 is V=15.3 mag. Brightest star in FOV has B=17.98, V=17.51, H=15.86 (2MASS J12592525+2759075).
J2000
J2000
B=16.8 H=12.7
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC4041 is V=14.8 mag. Brightest star in FOV has B=14.69, V=14.22, H=12.83 (2MASS J13003879+2801029).
J2000
J2000
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Brightest star in FOV has B=15.75, V=15.17, H=13.84 (2MASS J13002449+2800487).
J2000
J2000
B=15.75 H=13.84
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC4021 is V=14.8 mag. Brightest star in FOV has B=16.03, V=15.44, H=13.95 (2MASS J13001245+2800573).
J2000
J2000
B=16.0 H=12.0
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy 2MASX J12593141+2802478 is V=15.0 mag. Brightest star in FOV has B=17.27, V=16.66, H=15.01 (2MASS J12592653+2800239).
J2000
J2000
B=15.9 H=12.2
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC4040 is V=14.8 mag. Brightest star in FOV (western edge) has B=18.8, V=17.21, H=13.02 (2MASS J13003422+2804036).
J2000
J2000
B=15.1 H=12.3
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC4040 is V=14.8 mag. Brightest star in FOV (western edge) has B=18.8, V=17.21, H=13.02 (2MASS J13003422+2804036).
J2000
J2000
B=15.1 H=12.3
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy IC4026 is V=14.6 mag. Brightest star in FOV (eastern edge) has B=18.8, V=17.21, H=13.02 (2MASS J13003422+2804036).
J2000
J2000
B=15.5 H=11.8
CLUSTER OF GALAXIES
RICH CLUSTER
YES
Flux of brightest galaxy 2MASX J13001286+2804322 is V=15.2 mag. Brightest star in FOV has B=15.95, V=15.4, H=13.93 (2MASS J13001845+2802351).
J2000
J2000
B=16.3 H=12.4
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F336W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
SE corner
1451002839000
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false
3
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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:dark-utilization 0
:max-dark-utilization 1920
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false
3
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1451426536000
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false
3
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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false
3
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The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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SW corner
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The scheduling data was generated by CASM 23.2.
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The scheduling data was generated by CASM 23.2.
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The scheduling data was generated by CASM 23.2.
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The scheduling data was generated by CASM 23.2.
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The scheduling data was generated by CASM 23.2.
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The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Hst Same orient constraint links visits (15 16 17 19 20 21)
The scheduling data was generated by CASM 23.2.
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The scheduling data was generated by CASM 23.2.
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(Tic-Orbit
:proposal-id 14182
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:orbit-number 2
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:dark-offset NIL
:dark-utilization 0
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:low-sky "N"
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)
(Tic-Orbit
:proposal-id 14182
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)
false
3
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
NWN corner (horn)
1457094330000
232.1653881670743
(Tic-Visit
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)
(Tic-Obset
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)
(Tic-Orbit
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 14182
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:dark-offset NIL
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)
(Tic-Orbit
:proposal-id 14182
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:dark-offset NIL
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:max-dark-utilization 1920
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:pcs-visibility 3229
:pcs-gap 0
)
false
3
0
Hst Same orient constraint links visits (15 16 17 19 20 21)
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
NE corner
1464674820000
143.5
(Tic-Visit
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:coron NIL
)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
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:dark-offset NIL
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)
(Tic-Orbit
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:max-dark-utilization 1920
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)
false
3
0
NE corner
(Tic-Visit
:proposal-id 14182
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:trans-version "20160322"
:date "06-Jun-2016 11:44:01.0"
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)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
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)
(Tic-Orbit
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3229
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)
false
3
0
Hst Same orient constraint links visits (15 16 17 19 20 21)
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1464337642000
143.5
(Tic-Visit
:proposal-id 14182
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)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
:proposal-id 14182
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:orbit-number 2
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)
(Tic-Orbit
:proposal-id 14182
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:pcs-gap 0
)
false
3
0
Hst Same orient constraint links visits (15 16 17 19 20 21)
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
NNW corner
1464409225000
143.5
(Tic-Visit
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)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
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:dark-offset NIL
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)
(Tic-Orbit
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)
false
3
0