Program Number |
Principal Investigator |
Program Title |
13346 |
Thomas R. Ayres, University of Colorado at Boulder |
Advanced Spectral Library II: Hot Stars |
13354 |
Robert D. Mathieu, University of Wisconsin - Madison |
COS Spectroscopy of White Dwarf Companions to Blue Stragglers in NGC 188 |
13357 |
David J. Radburn-Smith, University of Washington |
Feeding Galaxies: Cold Accretion Through Warps |
13381 |
Marshall Perrin, Space Telescope Science Institute |
STIS Coronagraphy of Four Young Debris Disks Newly Uncovered from the NICMOS Archive |
13459 |
Tommaso L. Treu, University of California - Los Angeles |
The Grism Lens-Amplified Survey from Space {GLASS} |
13470 |
Julio Chaname, Pontificia Universidad Catolica de Chile |
Probing Cold Dark Matter Substructure with Wide Binaries in Dwarf Spheroidal Galaxies |
13472 |
Wendy L. Freedman, Carnegie Institution of Washington |
The Hubble Constant to 1%? STAGE 4: Calibrating the RR Lyrae PL relation at H-Band using HST and Gaia Parallax Stars |
13498 |
Jennifer Lotz, Space Telescope Science Institute |
HST Frontier Fields - Observations of MACSJ0717.5+3745 |
13671 |
Harald Ebeling, University of Hawaii |
Beyond MACS: A Snapshot Survey of the Most Massive Clusters of Galaxies at z>0.5 |
13677 |
Saul Perlmutter, University of California - Berkeley |
See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts |
13678 |
Adam Riess, The Johns Hopkins University |
The Fifth and Final Epoch |
13679 |
Lorenz Roth, Southwest Research Institute |
Europa's Water Vapor Plumes: Systematically Constraining their Abundance and Variability |
13692 |
William M. Grundy, Lowell Observatory |
Orbits and Physical Properties of Four Binary Transneptunian Objects |
13711 |
Abhijit Saha, National Optical Astronomy Observatory, AURA |
Establishing a Network of Next Generation SED standards with DA White Dwarfs |
13717 |
Lifan Wang, Texas A & M University |
Polarimetry of SN 2014J in M82 as a Probe of Its Dusty Environment |
13718 |
Julie Wardlow, University of Copenhagen, Niels Bohr Institute |
The nature and environment of the earliest dusty starburst galaxies |
13724 |
Todd J. Henry, Georgia State University Research Foundation |
Pinpointing the Characteristics of Stars and Not Stars --- VERSION 2014.1021 |
13729 |
Andy Lawrence, University of Edinburgh, Institute for Astronomy |
Slow-blue PanSTARRS transients : high amplification microlens events? |
13740 |
Daniel Stern, Jet Propulsion Laboratory |
Clusters Around Radio-Loud AGN: Spectroscopy of Infrared-Selected Galaxy Clusters at z>1.4 |
13745 |
Erik Tollerud, Yale University |
Resolving the Tip of the Red Giant Branch of Two New Candidate Local Group Dwarf Galaxies |
13760 |
Derck L. Massa, Space Science Institute |
Filling the gap --near UV, optical and near IR extinction |
13763 |
S. Thomas Megeath, University of Toledo |
WFC3 Spectroscopy of Faint Young Companions to Orion Young Stellar Objects |
13776 |
Michael D. Gregg, University of California - Davis |
Completing The Next Generation Spectral Library |
13789 |
Andrea Mehner, European Southern Observatory - Chile |
Essential UV Observations of Eta Carinae's Change of State |
13816 |
Misty C. Bentz, Georgia State University Research Foundation |
High-Resolution Imaging of Active Galaxies with Direct Black Hole Mass Measurements |
13819 |
Trent J. Dupuy, University of Texas at Austin |
Dynamical Masses for Free-Floating Planetary-Mass Binaries |
13841 |
Alexandre Gallenne, Universidad de Concepcion |
Accurate masses and distances of the binary Cepheids S Mus and SU Cyg |
13842 |
Frederick Hamann, University of Florida |
Testing the Youth and Transition Object Status of FeLoBAL Quasars |
13844 |
Bret Lehmer, The Johns Hopkins University |
Unveiling the Black Hole Growth Mechanisms in the Protocluster Environment at z ~ 3 |
13937 |
Amy Simon, NASA Goddard Space Flight Center |
Hubble 2020: Outer Planet Atmospheres Legacy (OPAL) Program |
14036 |
Laurent Lamy, Observatoire de Paris - Section de Meudon |
Post-equinox Uranus aurorae during a strong magnetosphere-solar wind shock interaction |