Initial submission for the "just in case" situation.
Second submission.
Third submission.
Fourth and hopefully the final submission.-748461294Assigned ID: 1767
----- Attempting Submission 1 (Fri Apr 09 00:32:53 GMT 2021) -----
HST Phase I Proposal 1767 successfully submitted.
Receipt: # 1767-1
----- Attempting Submission 2 (Fri Apr 09 20:08:10 GMT 2021) -----
HST Phase I Proposal 1767 successfully submitted.
Receipt: # 1767-2
----- Attempting Submission 3 (Fri Apr 09 21:30:03 GMT 2021) -----
HST Phase I Proposal 1767 successfully submitted.
Receipt: # 1767-3
----- Attempting Submission 4 (Fri Apr 09 23:35:49 GMT 2021) -----Initial submission.
Sep 16, 2022 - Split each of visits 03, 07, 09 into 3 single-orbit visits following PC's request. Also cut down orbit time for visits 07 and 09 by 2 min.227183275----- Attempting Submission 1 (Mon Jul 19 15:15:02 GMT 2021) -----
----- Attempting Submission 2 (Sat Sep 17 00:30:35 GMT 2022) -----Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: Constraining the Density and Properties of Dark MatterDetermination of the mass density profiles of dwarf galaxies (and specifically whether there is a central core or cusp) provides a critical test of both the properties of dark matter (DM) and the physics of cosmological structure formation. The nearby classical dwarf spheroidal galaxies (dSphs) of the Milky Way yield some of the best dynamical constraints. While large line-of-sight velocity datasets exist (some thousand stars per galaxy), interpretation is hindered by the well-known mass vs. velocity-anisotropy degeneracy of stellar dynamics. This can be resolved with proper motion (PM) measurements that yield 3-D velocity information. This is beyond the reach of Gaia, given the small velocity dispersions of dSphs and the absence of bright stars. HST is the only observatory that can advance this problem, given its combination of photometric depth, high spatial resolution, and long time baselines. We propose to obtain HST imaging of five previously imaged fields in the nearby Draco and Sculptor dSphs, to obtain high-accuracy PMs for thousands of stars in these galaxies. This provides a direct determination of their velocity anisotropy profiles, and combined with dynamical models, tightly constrains the slopes of their DM density profiles. The results will give unique constraints on both the nature of DM, and the physical mechanisms that shape DM density profiles in galaxies. No comparable measurements exist to date. The proposed program therefore shows how HST can still be used, after 30 years in orbit, to tackle unanswered fundamental questions in astrophysics.The primary goal of this program is to measure the internal proper motion kinematics of the two dwarf spheroidal galaxies Draco and Sculptor using multi-epoch HST imaging data. We will target 5 fields in total, 3 in Draco and 2 in Sculptor. Each target field will be observed for four orbits - three orbits will have the same telescope orientation as the older epoch observations, while the remaining one orbit will be observed with orientation rotated by an angle of 90 deg. The 90deg-rotated observations are for quantifying and correcting residual CTE effects. These telescope orientation conditions are added as special requirements for each visit.All investigators are members of the HSTPROMO group, led by co-I van der Marel, which has published numerous papers reporting proper motion measurements of dwarf galaxies, globular clusters, individual stars along stellar streams, and distant Milky Way (MW) halo stars.[*] PI Sohn has led many HST programs over the past decade for measuring proper motions of M31, bulk proper motions of dwarf spheroidal galaxies in the Milky Way halo (Leo I, Draco, and Sculptor), indivdual proper motions of stars along stellar streams such as Sagittarius, Orphan, and Lethe, distant Milky Way globular clusters, and M31 satellites NGC 147 and 185. He has been the PI for several of these programs, and will oversee this entire program. Co-PI del Pino-Molina is an expert in analysis of internal dynamics of dwarf galaxies in the Local Group. He will oversee the analysis of our multi-epoch data. Co-I Watkins is an expert in velocity anisotropy analysis and dynamical mass estimation, and has particularly published papers studying the internal kinematics and dynamics of MW globular clusters. Co-I Libralato is an expert of data reduction, proper-motion measurements and internal kinematics of globular clusters. Co-Is Besla, Patel, and van der Marel are experts in dynamical modeling of Local Group galaxies including both equilibrium and N-body modeling. Co-I Pawlowski is an expert on the topic of satellite galaxy phase-space correlations, in particular, planes of satellites and their use to predict proper motions, as well as the comparison of satellites systems and their orbits with cosmological simulations of structure formation. 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