Program Number |
Principal Investigator |
Program Title |
13024 |
John S. Mulchaey, Carnegie Institution of Washington |
A Public Snapshot Survey of Galaxies Associated with O VI and Ne VIII Absorbers |
13054 |
Theodore R. Gull, NASA Goddard Space Flight Center |
Constraining the evolutionary state of the hot, massive companion star and the wind-wind collision region in Eta Carinae |
13330 |
Bradley M Peterson, The Ohio State University |
Mapping the AGN Broad Line Region by Reverberation |
13375 |
Dougal Mackey, Australian National University |
Deep photometry of two accreted families of globular clusters in the remote M31 halo |
13386 |
Steven A. Rodney, The Johns Hopkins University |
Frontier Field Supernova Search |
13391 |
Nathan Smith, University of Arizona |
WFC3-IR Imaging of Dense, Embedded Outflows from Intermediate-Mass Protostars in Carina |
13463 |
Kailash C. Sahu, Space Telescope Science Institute |
Detecting and Measuring the Masses of Isolated Black Holes and Neutron Stars through Astrometric Microlensing |
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 |
13481 |
Emily Levesque, University of Colorado at Boulder |
Calibrating Multi-Wavelength Metallicity Diagnostics for Star-Forming Galaxies |
13498 |
Jennifer Lotz, Space Telescope Science Institute |
HST Frontier Fields - Observations of MACSJ0717.5+3745 |
13639 |
Matthew Bayliss, Harvard University |
Resolving Lyman-alpha Emission On Physical Scales < 270 pc at z > 4 |
13686 |
Adam Riess, The Johns Hopkins University |
The Longest Period Cepheids, a bridge to the Hubble Constant |
13691 |
Wendy L. Freedman, Carnegie Institution of Washington |
CHP-II: The Carnegie Hubble Program to Measure Ho to 3% Using Population II |
13726 |
Paul Kalas, University of California - Berkeley |
Scattered light imaging of Fomalhaut's ice line belt to understand dynamical upheavals in planetary systems |
13935 |
Howard E. Bond, The Pennsylvania State University |
The Nature of SPIRITS Intermediate-Luminosity Mid-IR Transients |