0
Assigned ID: 1117
----- Attempting Submission 1 (Sat Apr 08 00:34:52 GMT 2017) -----
HST Phase I Proposal 1117 (massive-gc.apt) successfully submitted.
Receipt: # 1117-1
Resubmission just for 2nd orbit of Visit 21 - now cloned to one orbit in Visit 71
(had to decrease exposure times to make it fit).
Thanks!
4/1/19 ROYLE - Added ORIENT to repeat visit 71 to match execution of visit 21
4/1/19 Blakeslee - put first exposure back to 84 sec and readjusted the rest.
1074168365
----- Attempting Submission 1 (Sat Jul 01 02:42:39 GMT 2017) -----
HST Phase II Proposal 15265 (15265_v1.apt) successfully submitted.
Receipt: # 15265-1
----- Attempting Submission 2 (Mon Jul 17 15:31:32 GMT 2017) -----
HST Phase II Proposal 15265 (15265_v3.apt) successfully submitted.
Receipt: # 15265-2
----- Attempting Submission 3 (Wed Jul 19 20:24:11 GMT 2017) -----
HST Phase II Proposal 15265 (15265_v3.apt) successfully submitted.
Receipt: # 15265-3
----- Attempting Submission 4 (Fri Sep 08 03:40:38 GMT 2017) -----
HST Phase II Proposal 15265 (15265_v5.apt) successfully submitted.
Receipt: # 15265-4
----- Attempting Submission 5 (Sat Sep 09 02:31:40 GMT 2017) -----
----- Attempting Submission 6 (Fri Mar 22 20:45:58 GMT 2019) -----
----- Attempting Submission 7 (Mon Apr 01 14:29:53 GMT 2019) -----
----- Attempting Submission 8 (Mon Apr 01 20:44:53 GMT 2019) -----
I just cloned the Visit 21, orbit 2 observation - I didn't change the flash, so should still be the same.
Adjusted time of 1st short exposure.
MASSIVE+: The Growth Histories of MASSIVE Survey Galaxies from their Globular Cluster Colors
The MASSIVE survey is targeting the ~100 most massive galaxies within 108 Mpc that are visible in the northern sky. These most massive galaxies in the present-day universe reside in a surprisingly wide variety of environments, from rich clusters to fossil groups to near isolation. We propose to use WFC3/UVIS and ACS to carry out a deep imaging study of the globular cluster populations around a selected subset of the MASSIVE targets. Though much is known about GC systems of bright galaxies in rich clusters, we know surprisingly little about the effects of environment on these systems. The MASSIVE sample provides a golden opportunity to learn about the systematics of GC systems and what they can tell us about environmental drivers on the evolution of the highest mass galaxies. The most pressing questions to be addressed include: (1) Do isolated giants have the same constant mass fraction of GCs to total halo mass as BCGs of similar luminosity? (2) Do their GC systems show the same color (metallicity) distribution, which is an outcome of the mass spectrum of gas-rich halos during hierarchical growth? (3) Do the GCs in isolated high-mass galaxies follow the same radial distribution versus metallicity as in rich environments (a test of the relative importance of growth by accretion)? (4) Do the GCs of galaxies in sparse environments follow the same mass function? Our proposed second-band imaging will enable us to secure answers to these questions and add enormously to the legacy value of existing HST imaging of the highest mass galaxies in the universe.
WFC3/UVIS F475X imaging of a sample of 15 galaxies selected from the MASSIVE Survey.
9 galaxies have 1 orbit each [WFC3/UVIS/F475X prime + ACS/F475W par]
6 galaxies have 2 orbits each; [extra orbit is: WFC3/IR/F110W prime + ACS/F814 par]
total of 21 orbits.
Thus, all orbits now have parallel imaging with ACS/WFC.
Stellar Populations
Galaxies and the IGM
6
false
false
false
false
false
false
false
SUPPORTED
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
GALAXY
ELLIPTICAL
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
WFC3/UVIS
Imaging
No
No
F475X
WFC3/UVIS
Imaging
No
No
F475X
WFC3/UVIS
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No
No
F475X
WFC3/UVIS
Imaging
No
No
F475X
WFC3/UVIS
Imaging
No
No
F475X
WFC3/UVIS
Imaging
No
No
F475X
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No
No
F475X
WFC3/UVIS
Imaging
No
No
F475X
WFC3/UVIS
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No
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F475X
WFC3/IR
Imaging
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No
F110W
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No
F475X
WFC3/IR
Imaging
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No
F110W
WFC3/UVIS
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No
F475X
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Imaging
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No
F110W
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Imaging
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No
F475X
WFC3/IR
Imaging
No
No
F110W
WFC3/UVIS
Imaging
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No
F475X
WFC3/IR
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No
No
F110W
WFC3/UVIS
Imaging
No
No
F475X
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Imaging
No
No
F475X
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No
F110W
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No
F475W
ACS/WFC
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No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
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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
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
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No
F814W
ACS/WFC
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No
F475W
ACS/WFC
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No
F814W
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No
F475W
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No
F814W
ACS/WFC
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No
No
F475W
ACS/WFC
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No
F814W
ACS/WFC
Imaging
No
No
F475W
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No
No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
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No
F475W
ACS/WFC
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No
F814W
ACS/WFC
Imaging
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No
F475W
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F814W
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F475W
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F814W
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POS-TARG
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LINE
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72.9884
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WFC3-IR-DITHER-BOX-MIN
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This is a re-do of 2nd orbit of Visit 21.
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