Program Number | Principal Investigator | Program Title |
---|---|---|
12034 | James C. Green, University of Colorado at Boulder | COS-GTO: Brown Dwarf Activity Part 2 |
12109 | Julianne Dalcanton, University of Washington | A Panchromatic Hubble Andromeda Treasury - I |
12111 | Julianne Dalcanton, University of Washington | A Panchromatic Hubble Andromeda Treasury - I |
12471 | Dawn K. Erb, University of Wisconsin - Milwaukee | The Bottom of the Iceberg: Faint z~2 Galaxies and the Enrichment of the IGM |
12488 | Mattia Negrello, Open University | SNAPshot observations of gravitational lens systems discovered via wide-field Herschel imaging |
12528 | Philip Massey, Lowell Observatory | Probing the Nature of LBVs in M31 and M33: Blasts from the Past |
12568 | Matthew A. Malkan, University of California - Los Angeles | WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time |
12575 | Anthony H. Gonzalez, University of Florida | New Constraints on Intragroup Light and the Baryon Budget in Galaxy Groups |
12595 | Michael Eracleous, The Pennsylvania State University | Unraveling the LINER Conspiracy |
12662 | Oleg Y. Gnedin, University of Michigan | Hypervelocity Stars as Unique Probes of the Galactic Center and Outer Halo |
12788 | Marc Postman, Space Telescope Science Institute | Through a Lens, Darkly - New Constraints on the Fundamental Components of the Cosmos |
12813 | Brian Schmidt, Australian National University | Network of 13 high precision STIS spectrophotometric standards for ground based surveys |
12861 | Xiaohui Fan, University of Arizona | Morphologies of the Most UV luminous Lyman Break Galaxies at z~3 |
12866 | Mark Swinbank, University of Durham | A Morphological Study of ALMA Identified Sub-mm Galaxies with HST/WFC3 |
12870 | Boris T. Gaensicke, The University of Warwick | The mass and temperature distribution of accreting white dwarfs |
12884 | Harald Ebeling, University of Hawaii | A Snapshot Survey of The Most Massive Clusters of Galaxies |
12903 | Luis C. Ho, Carnegie Institution of Washington | The Evolutionary Link Between Type 2 and Type 1 Quasars |
12928 | Alaina L. Henry, Oak Ridge Associated Universities | Gaseous outflows from low mass galaxies: Understanding local laboratories for high redshift star formation |
12939 | Elena Sabbi, Space Telescope Science Institute - ESA | Hubble Tarantula Treasury Project {HTTP: unraveling Tarantula's web} |
12940 | Philip Massey, Lowell Observatory | The Unevolved Massive Star Content of the Magellanic Clouds |
12969 | Peter Garnavich, University of Notre Dame | Global Properties Are Not Enough: Probing the Local Environments of Type Ia Supernovae |
12982 | Nicolas Lehner, University of Notre Dame | Are the Milky Way's High Velocity Clouds Fuel for Star Formation or for the Galactic Corona? |
12996 | Christopher Johns-Krull, Rice University | Exploring the Role of Stellar Magnetic Fields in Accretion and Outflows from Young Stars using the Hot Emission Lines of Herbig Ae/Be Stars |
13003 | Michael D. Gladders, University of Chicago | Resolving the Star Formation in Distant Galaxies |
13017 | Timothy M. Heckman, The Johns Hopkins University | UV Spectroscopy of Lyman Break Galaxy Analogs: A Local Window on the Early Universe |
13025 | Andrew J. Levan, The University of Warwick | Unveiling the progenitors of the most luminous supernovae |
13029 | Alex V. Filippenko, University of California - Berkeley | A Snapshot Survey of the Sites of Recent, Nearby Supernovae |
13033 | Jason Tumlinson, Space Telescope Science Institute | COS-Halos: New FUV Measurements of Baryons and Metals in the Inner Circumgalactic Medium |
13046 | Robert P. Kirshner, Harvard University | RAISIN: Tracers of cosmic expansion with SN IA in the IR |
13048 | Jay Strader, Michigan State University | The First Unambiguous Detection of a Distinct Metal-poor Stellar Halo in a Massive Early-type Galaxy |
GO 12105, 12107: A Panchromatic Hubble Andromeda Treasury
M31: the Andromeda spiral galaxy |
M31, the Andromeda galaxy, is the nearest large spiral system to the Milky Way (d ~ 700 kpc), and, with the Milky Way, dominates the Local Group. The two galaxies are relatively similar, with M31 likely the larger system; thus, Andromeda provides the best opportunity for a comparative assessment of the structural properties of the Milky Way. Moreover, while M31 is (obviously) more distant, our external vantage point can provide crucial global information that complements the detailed data that we can acquire on individual members of the stellar populations of the Milky Way. With the advent on the ACS and, within the last 2 years, WFC3 on HST, it has become possible to resolve main sequence late-F and G dwarfs, permitting observations that extend to sub-solar masses in M31's halo and disk. Initially, most attention focused on the extended halo of M31 (eg the Cycle 15 program GO 10816 ), with deep imaging within a limited number of fields revealing the complex metallicity structure within that population. With the initiation of the present Multi-Cycle Treasury program, attention switches to the M31 disk. "PHAT" is conducting a multi-waveband survey of approximately one third of disk and bulge, focusing on the north-east quadrant. Observations have been taken over Cycles 18, 19 and 20, and are providing a thorough census of upper main-sequence stars, open clusters, associations and star forming regions, matching the stellar distribution against the dust and gas distribution. |
GO 12662: Hypervelocity Stars as Unique Probes of the Galactic Center and Outer Halo
GO 12870: The mass and temperature distribution of accreting white dwarfs