Program Number |
Principal Investigator |
Program Title |
13472 |
Wendy L. Freedman, University of Chicago |
The Hubble Constant to 1%? STAGE 4: Calibrating the RR Lyrae PL relation at H-Band using HST and Gaia Parallax Stars |
13646 |
Ryan Foley, University of Illinois at Urbana - Champaign |
Understanding the Progenitor Systems, Explosion Mechanisms, and Cosmological Utility of Type Ia Supernovae |
13654 |
Matthew Hayes, Stockholm University |
Ultraviolet Spectroscopy of the Extended Lyman Alpha Reference Sample |
13655 |
Matthew Hayes, Stockholm University |
How Lyman alpha bites/beats the dust |
13656 |
Matthew Hayes, Stockholm University |
Unveiling the Dark Baryons: The First Imaging of Circumgalactic OVI in Emission |
13659 |
Karin Sandstrom, University of California - San Diego |
A New View of Dust at Low Metallicity: The First Maps of SMC Extinction Curves |
13661 |
Matthew Auger, University of Cambridge |
A SHARP View of the Structure and Evolution of Normal and Compact Early-type Galaxies |
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 |
13679 |
Lorenz Roth, Royal Institute of Technology |
Europa's Water Vapor Plumes: Systematically Constraining their Abundance and Variability |
13682 |
Pieter van Dokkum, Yale University |
Distances and stellar populations of seven low surface brightness galaxies in the field of M101 |
13686 |
Adam Riess, The Johns Hopkins University |
The Longest Period Cepheids, a bridge to the Hubble Constant |
13691 |
Wendy L. Freedman, University of Chicago |
CHP-II: The Carnegie Hubble Program to Measure Ho to 3% Using Population II |
13692 |
William M. Grundy, Lowell Observatory |
Orbits and Physical Properties of Four Binary Transneptunian Objects |
13695 |
Benne W. Holwerda, Sterrewacht Leiden |
STarlight Absorption Reduction through a Survey of Multiple Occulting Galaxies (STARSMOG) |
13696 |
Benne W. Holwerda, Sterrewacht Leiden |
The Anemic Stellar Halo of M101 |
13704 |
Steven G. Parsons, Valparaiso University |
Testing the single degenerate channel for supernova Ia |
13732 |
Anna Nierenberg, The Ohio State University |
Detecting dark matter substructure with narrow line lensing |
13748 |
Luigi R. Bedin, Osservatorio Astronomico di Padova |
Astrometric search for Planets in the closest Brown Dwarf Binary system Luhman 16AB |
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 |
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) |
13783 |
George G. Pavlov, The Pennsylvania State University |
Thermal evolution of old neutron stars |
13792 |
Rychard Bouwens, Universiteit Leiden |
A Complete Census of the Bright z~9-10 Galaxies in the CANDELS Data Set |
13816 |
Misty C. Bentz, Georgia State University Research Foundation |
High-Resolution Imaging of Active Galaxies with Direct Black Hole Mass Measurements |
13826 |
Massimo Robberto, Space Telescope Science Institute |
The Orion Nebula Cluster as a Paradigm of Star Formation |
13868 |
Dale D. Kocevski, Colby College |
Are Compton-Thick AGN the Missing Link Between Mergers and Black Hole Growth? |
13871 |
Pascal Oesch, Yale University |
A Spectroscopic Redshift for the Most Luminous Galaxy Candidate at z~10 |
13872 |
Pascal Oesch, Yale University |
The GOODS UV Legacy Fields: A Full Census of Faint Star-Forming Galaxies at z~0.5-2 |
13876 |
Howard E. Bond, The Pennsylvania State University |
HST Observations of Astrophysically Important Visual Binaries |
13950 |
Andrew S. Fruchter, Space Telescope Science Institute |
The Astrophysics of the Most Energetic Gamma-Ray Bursts |
14058 |
Karen M. Leighly, University of Oklahoma Norman Campus |
Using the WPVS 007 Occultation Event to Constrain the Astrophysics of Quasar Outflows |