0
Assigned ID: 249
----- Attempting Submission 1 (Thu Apr 09 20:14:02 GMT 2015) -----
HST Phase I Proposal 249 (apt_mcs.apt) successfully submitted.
Receipt: # 249-1
Resubmission of the proposal is due to the orientation requirement problem for some targets/visits.
The orinetation requirement were modifiyed for some visits/targets.
Dues to the duplication of F336W filters in two GO programs, F336W in 14069 have been replaced
by F555W - "DDR 81762 for the WFC programs 14069 and 14204 on Aug 12, 2015"
Target chang requiest: Visit 11 - ngc361 is replaced by ngc1978
Change Request 85230, approved by TTRB.
Resubmission is due to the changes in ORIENTAT(U3) in order to enlarge
the Plan Window and early scheduling.
1627009897
----- Attempting Submission 1 (Thu Jul 23 21:21:11 GMT 2015) -----
----- Attempting Submission 2 (Tue Aug 18 18:41:40 GMT 2015) -----
----- Attempting Submission 3 (Thu Aug 27 18:49:54 GMT 2015) -----
----- Attempting Submission 4 (Tue Oct 06 18:24:40 GMT 2015) -----
----- Attempting Submission 5 (Thu Jul 28 19:30:12 GMT 2016) -----
----- Attempting Submission 6 (Fri Jul 29 16:23:20 GMT 2016) -----
Searching For Multiple Populations in Massive Young and Intermediate Age Clusters
We propose to obtain imaging of 12 massive clusters within the LMC/SMC, spanning a wide range of ages (100 Myr - 10 Gyr), in order to search for abundance spreads (i.e. multiple populations) within them. While all ancient globular clusters (GCs) studied to date, in the necessary detail, possess multiple populations, no massive (>10^5 Msun) young (< 1 Gyr) or intermediate (1-8 Gyr) age clusters have been found with abundance spreads. This raises the fundamental question: what controls whether a cluster will host multiple populations? The standard suggestion is that cluster mass is the crucial parameter, although recent results on the initial masses of GCs have called this into question. An alternative view is that GC formation was fundamentally different than the formation of other (< 10 Gyr) massive clusters. The proposed observations will definitively address whether age or mass is the crucial parameter controlling the appearance of multiple populations. The proposed sample occupies a critical region of parameter space (age/mass) where there are no Milky Way counterparts.
We propose to obtain imaging of 12 massive star clusters within the LMC/SMC, spanning a wide range of ages (0.1 - 10 Gyr), in order to search for elemental abundance spreads and multiple populations. The clusters will be observed in the F343N, F336W and F438W WFC3/UVIS filters,
which will provide accurate color-magnitude diagrams (CMD) for studies of these phenomena.
A CMD for such a large range of stellar ages covers everything from red and very bright giants down to the main sequence stars of various brightness and colors. To reach our science goals, it is crucial not to saturate the bright giants by using a short exposure and to reach a sufficient depth beyond the main-sequence turn-off using long exposures. Therefore, for each cluster, a short exposure and two or three long exposures in each filter are required. To cover the gap between the two WFC3/UVIS CCD chips, we use two dithered pointings. In order to maximize the overlap, we also require a specific orientation to match the orientation of those target clusters which have archival observations with the WFC3/UVIS. This orientation is specified in the Visit Orientation Requirement for these clusters/visits as follows: Visit3 - ngc1856, Min=324, Max=334;
Visit4 - ngc419, Min=307, Max=317; Visit5-ngc1783, Min=298, Max=308;
Visit6 - ngc1806, Min=297, Max=307; Visit7 - ngc1846, Min=122, Max=132;
Visit12 - ngc121, Min=215 to Max=225.
RESOLVED STELLAR POPULATIONS
12
false
false
false
false
false
false
SUPPORTED
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
Coordinates were selected so as to yield good overlap with existing ACS images.
J2000
J2000
STELLAR CLUSTER
GLOBULAR CLUSTER
OPEN CLUSTER
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F438W
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
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No
F336W
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Imaging
No
No
F438W
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
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No
No
F438W
WFC3/UVIS
Imaging
No
No
F343N
WFC3/UVIS
Imaging
No
No
F336W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/UVIS
Imaging
No
No
F343N
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Visit 11 - ngc361 is replaced by ngc1978
Change Request 85230, approved by TTRB
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