0
Assigned ID: 740
----- Attempting Submission 1 (Fri Apr 11 19:58:31 GMT 2014) -----
HST Phase I Proposal 740 (2014_03_HST_Andies_Shallow.apt) successfully submitted.
----- Attempting Submission 2 (Fri Apr 11 20:05:27 GMT 2014) -----
----- Attempting Submission 3 (Sun Apr 13 11:11:52 GMT 2014) -----
0
----- Attempting Submission 1 (Thu Jul 24 08:09:48 GMT 2014) -----
----- Attempting Submission 2 (Fri Sep 12 20:44:06 GMT 2014) -----
A bug in APT stalls the generation of the sky charts when clicking "Target Confirmation", preventing me from running this tool.
Fellowship of the Andromeda Dwarf Galaxies: A Census of their Extended Star Formation Histories
We propose an efficient HST/ACS imaging survey of all 19 Andromeda satellite dwarf spheroidal galaxies that have not yet been observed with HST. The resulting color-magnitude diagrams will reach S/N=5-10 2 magnitude below the horizontal branch and will provide (a) precise distances to each of the galaxies and (b) well-constrained star formation histories (SFHs) for ages younger than ~8-10 Gyr ago. Neither of these goals can be achieved to the needed level of precision from ground based observations. Recent studies of the structural and age distributions of Andromeda's satellites hint at significant and systematic differences with properties of the Milky Way (MW) satellites, e.g., a co-rotating planar satellite structure and systematically larger intermediate age populations. But both suffer from uncertainties due the limitations of even the largest ground-based telescope (Subaru, LBT). Our proposed observations will provide an efficient way to test for these differences by tightly constraining intermediate age SFHs and improving distance determinations for all 19 systems. The discoveyr of systematic age differences with the MW group would have significant implications for our understanding of satellite systems, their relationship to a host galaxy, and cosmological modeling of low mass galaxies, all of which are exclusively based on observations of the MW companions.
The aim of this proposal is to gather two-band photometry of a series of dwarf galaxies, satellites of Andromeda, in order to build deep color-magnitude diagrams of theses stellar systems with ACS and a parallel WFC3 pointing. The observations are straightforward, with a single orbit spent on every target being split between 2 F606W and 2 F814W sub-exposures (to allow for cosmic ray removal). In parallel, a single exposure per filter is obtained with WFC3.
RESOLVED STELLAR POPULATIONS
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