Program Number |
Principal Investigator |
Program Title |
13665 |
Bjoern Benneke, California Institute of Technology |
Exploring the Diversity of Exoplanet Atmospheres in the Super-Earth Regime |
13715 |
Jennifer Sokoloski, Columbia University in the City of New York |
Imaging Spectroscopy of the Gamma-Ray Nova V959 Mon |
13740 |
Daniel Stern, Jet Propulsion Laboratory |
Clusters Around Radio-Loud AGN: Spectroscopy of Infrared-Selected Galaxy Clusters at z>1.4 |
13769 |
Klaus Werner, Eberhard Karls Universitat, Tubingen |
Trans-iron group elements in hot helium-rich white dwarfs |
13794 |
John T. Clarke, Boston University |
Seasonal Dependence of the Escape of Water from the Martian Atmosphere |
13845 |
Adam Muzzin, University of Cambridge |
Resolved H-alpha Maps of Star-forming Galaxies in Distant Clusters: Towards a Physical Model of Satellite Galaxy Quenching |
13868 |
Dale D. Kocevski, Colby College |
Are Compton-Thick AGN the Missing Link Between Mergers and Black Hole Growth? |
14057 |
Fabien Grise, Universite de Strasbourg I |
Changes in the X-ray irradiation of an ultraluminous X-ray source |
14071 |
Sanchayeeta Borthakur, The Johns Hopkins University |
How are HI Disks Fed? Probing Condensation at the Disk-Halo Interface |
14076 |
Boris T. Gaensicke, The University of Warwick |
An HST legacy ultraviolet spectroscopic survey of the 13pc white dwarf sample |
14077 |
Boris T. Gaensicke, The University of Warwick |
The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps |
14080 |
Anne Jaskot, Smith College |
LyC, Ly-alpha, and Low Ions in Green Peas: Diagnostics of Optical Depth, Geometry, and Outflows |
14095 |
Gabriel Brammer, Space Telescope Science Institute - ESA |
Calibrating the Dusty Cosmos: Extinction Maps of Nearby Galaxies |
14096 |
Dan Coe, Space Telescope Science Institute - ESA |
RELICS: Reionization Lensing Cluster Survey |
14122 |
Lise Christensen, University of Copenhagen, Niels Bohr Institute |
Unveiling stellar populations in absorption-selected galaxies |
14127 |
Michele Fumagalli, Durham Univ. |
First Measurement of the Small Scale Structure of Circumgalactic Gas via Grism Spectra of Close Quasar Pairs |
14138 |
Kohji Tsumura, FRIS, Tohoku University |
Absolute Measurement of the Cosmic Near-Infrared Background Using Eclipsed Galilean Satellites as Occulters |
14148 |
Eiichi Egami, University of Arizona |
Near-IR Imaging of Three Spectacular Lensed Submillimeter Galaxies Discovered by the Herschel Lensing Survey |
14172 |
Brendan Bowler, University of Texas at Austin |
Imaging Accreting Protoplanets in the Young Cluster IC 348 |
14178 |
Matthew A. Malkan, University of California - Los Angeles |
WFC3 Infrared Spectroscopic Parallel Survey: The WISP Deep Fields |
14189 |
Adam S. Bolton, University of Utah |
Quantifying Cold Dark Matter Substructure with a Qualitatively New Gravitational Lens Sample |
14205 |
Andrew B. Newman, Carnegie Institution of Washington |
Early Quiescent Galaxies Under the Magnifying Glass |
14216 |
Robert P. Kirshner, Harvard University |
RAISIN2: Tracers of cosmic expansion with SN IA in the IR |
14219 |
John P. Blakeslee, Dominion Astrophysical Observatory |
Homogeneous Distances and Central Profiles for MASSIVE Survey Galaxies with Supermassive Black Holes |
14227 |
Casey Papovich, Texas A & M University |
The CANDELS Lyman-alpha Emission At Reionization (CLEAR) Experiment |
14231 |
Ian U. Roederer, University of Michigan |
The First Detections of Phosphorus, Sulphur, and Zinc in a Bona-Fide Second-Generation Star |
14271 |
Walter Peter Maksym, Smithsonian Institution Astrophysical Observatory |
Mapping the Radiative and Kinetic History of Fading AGNs |
14327 |
Saul Perlmutter, University of California - Berkeley |
See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts |
14340 |
Alexandre Gallenne, Universidad de Concepcion |
Accurate masses and distances of the binary Cepheids S Mus and SU Cyg |
14358 |
Roberto Assef, Diego Portales University |
Extremely Luminous Dusty Quasars with Unobscured UV Emission: Dual AGN or Extreme Single AGN Systems? |