Program Number |
Principal Investigator |
Program Title |
13651 |
Amy Kathryn Furniss, California State University - East Bay |
Disentangling Signatures of Ultra-high-energy Cosmic Rays from a Unique Gamma-ray Blazar |
13691 |
Wendy L. Freedman, University of Chicago |
CHP-II: The Carnegie Hubble Program to Measure Ho to 3% Using Population II |
13711 |
Abhijit Saha, National Optical Astronomy Observatory, AURA |
Establishing a Network of Next Generation SED standards with DA White Dwarfs |
13763 |
S. Thomas Megeath, University of Toledo |
WFC3 Spectroscopy of Faint Young Companions to Orion Young Stellar Objects |
13767 |
Michele Trenti, University of Melbourne |
Bright Galaxies at Hubble's Detection Frontier: The redshift z~9-10 BoRG pure-parallel survey |
13779 |
Sangeeta Malhotra, Arizona State University |
The Faint Infrared Grism Survey (FIGS) |
13801 |
Varsha Kulkarni, University of South Carolina Research Foundation |
Probing Structure in Cold Gas at z <~ 1 with Gravitationally Lensed Quasar Sightlines |
14054 |
Ehud Behar, Technion-Israel Institute of Technology |
Tracking Down the Ionized Outflow of NGC 7469 |
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 |
14096 |
Dan Coe, Space Telescope Science Institute - ESA |
RELICS: Reionization Lensing Cluster Survey |
14119 |
Luciana C. Bianchi, The Johns Hopkins University |
Understanding Stellar Evolution of Intermediate-Mass Stars from a New Sample of SiriusB-Like Binaries |
14127 |
Michele Fumagalli, Durham Univ. |
First Measurement of the Small Scale Structure of Circumgalactic Gas via Grism Spectra of Close Quasar Pairs |
14133 |
David Polishook, Weizmann Institute of Science |
Establishing an evolutionary sequence for disintegrated minor planets |
14138 |
Kohji Tsumura, FRIS, Tohoku University |
Absolute Measurement of the Cosmic Near-Infrared Background Using Eclipsed Galilean Satellites as Occulters |
14141 |
Guy Worthey, Washington State University |
NGSL Extension 1. Hot Stars and Evolved Stars |
14149 |
Alex V. Filippenko, University of California - Berkeley |
Continuing a Snapshot Survey of the Sites of Recent, Nearby Supernovae |
14163 |
Mickael Rigault, Humboldt Universitat zu Berlin |
Honing Type Ia Supernovae as Distance Indicators, Exploiting Environmental Bias for H0 and w. |
14171 |
Guangtun Zhu, The Johns Hopkins University |
Characterizing the Circumgalactic Medium of Luminous Red Galaxies |
14189 |
Adam S. Bolton, University of Utah |
Quantifying Cold Dark Matter Substructure with a Qualitatively New Gravitational Lens Sample |
14212 |
Karl Stapelfeldt, NASA Goddard Space Flight Center |
A Snapshot Imaging Survey of Spitzer-selected Young Stellar Objects in Nearby Star Formation Regions*.t23 |
14219 |
John P. Blakeslee, Dominion Astrophysical Observatory |
Homogeneous Distances and Central Profiles for MASSIVE Survey Galaxies with Supermassive Black Holes |
14241 |
Daniel Apai, University of Arizona |
Cloud Atlas: Vertical Cloud Structure and Gravity in Exoplanet and Brown Dwarf Atmospheres |
14249 |
Roberto Mignani, INAF, Istituto di Astrofisica Spaziale e Fisica |
The old pulsar PSR J0108-1431, a key target to understand the long-term evolution of neutron stars |
14260 |
Drake Deming, University of Maryland |
A Metallicity and Cloud Survey of Exoplanetary Atmospheres Prior to JWST |
14262 |
Knud Jahnke, Max-Planck-Institut fur Astronomie, Heidelberg |
Are the fastest growing black holes at z=2 caused by major galaxy mergers? |
14268 |
Nicolas Lehner, University of Notre Dame |
Project AMIGA: Mapping the Circumgalactic Medium of Andromeda |
14327 |
Saul Perlmutter, University of California - Berkeley |
See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts |