Program Number |
Principal Investigator |
Program Title |
13297 |
Giampaolo Piotto, Universita degli Studi di Padova |
The HST Legacy Survey of Galactic Globular Clusters: Shedding UV Light on Their Populations and Formation |
13498 |
Jennifer Lotz, Space Telescope Science Institute |
HST Frontier Fields - Observations of MACSJ0717.5+3745 |
13653 |
Caitlin Ann Griffith, University of Arizona |
Elementary Abundances of Planetary Systems |
13655 |
Matthew Hayes, Stockholm University |
How Lyman alpha bites/beats the dust |
13657 |
Jeyhan Kartaltepe, National Optical Astronomy Observatory, AURA |
Probing the Most Luminous Galaxies in the Universe at the Peak of Galaxy Assembly |
13662 |
Aaron J. Barth, University of California - Irvine |
Measuring the Black Hole Mass in the Brightest Cluster Galaxy NGC 1275 |
13677 |
Saul Perlmutter, University of California - Berkeley |
See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts |
13679 |
Lorenz Roth, Royal Institute of Technology |
Europa's Water Vapor Plumes: Systematically Constraining their Abundance and Variability |
13690 |
Tanio Diaz-Santos, California Institute of Technology |
Tracking the Obscured Star Formation Along the Complete Evolutionary Merger Sequence of LIRGs |
13691 |
Wendy L. Freedman, University of Chicago |
CHP-II: The Carnegie Hubble Program to Measure Ho to 3% Using Population II |
13695 |
Benne W. Holwerda, Sterrewacht Leiden |
STarlight Absorption Reduction through a Survey of Multiple Occulting Galaxies (STARSMOG) |
13697 |
Vianney Lebouteiller, CEA/DSM/Irfu/Service d'Astrophysique - Laboratoire AIM |
Does star formation proceed differently in metal-poor galaxies? |
13703 |
Lida Oskinova, Universitat Potsdam |
The donor star winds in High-Mass X-ray Binaries |
13711 |
Abhijit Saha, National Optical Astronomy Observatory, AURA |
Establishing a Network of Next Generation SED standards with DA White Dwarfs |
13721 |
Robert A. Benjamin, University of Wisconsin - Whitewater |
The Windy Milky Way Galaxy |
13723 |
Bruce Elmegreen, IBM T.J. Watson Research Center |
Multiband Observations of a Local Tadpole Galaxy |
13728 |
Steven Kraemer, Catholic University of America |
Do QSO2s have Narrow Line Region Outflows? Implications for quasar-mode feedback |
13734 |
Veronique Petit, Florida Institute of Technology |
Probing the extreme wind confinement of the most magnetic O star with COS spectroscopy |
13741 |
Thaisa Storchi-Bergmann, Universidade Federal do Rio Grande do Sul |
Constraining the structure of the Narrow-Line Region of nearby QSO2s |
13750 |
John M. Cannon, Macalester College |
Fundamental Parameters of the SHIELD II Galaxies |
13760 |
Derck L. Massa, Space Science Institute |
Filling the gap --near UV, optical and near IR extinction |
13761 |
Stephan Robert McCandliss, The Johns Hopkins University |
High efficiency SNAP survey for Lyman alpha emitters at low redshift |
13773 |
Rupali Chandar, University of Toledo |
H-alpha LEGUS: Unveiling the Interplay Between Stars, Star Clusters, and Ionized Gas |
13776 |
Michael D. Gregg, University of California - Davis |
Completing The Next Generation Spectral Library |
13779 |
Sangeeta Malhotra, Arizona State University |
The Faint Infrared Grism Survey (FIGS) |
13805 |
Kurt D. Retherford, Southwest Research Institute |
Io's Atmosphere Silhouetted in Transit by Jupiter Lyman-alpha |
13826 |
Massimo Robberto, Space Telescope Science Institute |
The Orion Nebula Cluster as a Paradigm of Star Formation |
13845 |
Adam Muzzin, Sterrewacht Leiden |
Resolved H-alpha Maps of Star-forming Galaxies in Distant Clusters: Towards a Physical Model of Satellite Galaxy Quenching |
13858 |
Annalisa De Cia, Weizmann Institute of Science |
The environment of the rarest and most energetic supernovae: do pair-instability explosions exist in the nearby Universe? |
13872 |
Pascal Oesch, Yale University |
The GOODS UV Legacy Fields: A Full Census of Faint Star-Forming Galaxies at z~0.5-2 |
13943 |
Amy E. Reines, University of Michigan |
Probing the Growth of Massive Black Holes in Dwarf Galaxies with Chandra and HST |