Program Number |
Principal Investigator |
Program Title |
13504 |
Jennifer Lotz, Space Telescope Science Institute |
HST Frontier Fields - Observations of MACSJ1149.5+2223 |
13642 |
Nathalie Degenaar, University of Cambridge |
The evolutionary link between low-mass X-ray binaries and millisecond radio pulsars |
13647 |
Ryan Foley, University of Illinois at Urbana - Champaign |
Testing the Standardizability of Type Ia Supernovae with the Cepheid Distance of a Twin Supernova |
13652 |
Boris T. Gaensicke, The University of Warwick |
The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps |
13667 |
Marc W. Buie, Southwest Research Institute |
Observations of the Pluto System During the New Horizons Encounter Epoch |
13668 |
Marc W. Buie, Southwest Research Institute |
Deep Search for Small Satellites of Eris and Makemake |
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 |
13689 |
Aleksandar M. Diamond-Stanic, University of Wisconsin - Madison |
How Compact is the Stellar Mass in Eddington-Limited Starbursts? |
13690 |
Tanio Diaz-Santos, Universidad Diego Portales |
Tracking the Obscured Star Formation Along the Complete Evolutionary Merger Sequence of LIRGs |
13691 |
Wendy L. Freedman, University of Chicago |
CHP-II: The Carnegie Hubble Program to Measure Ho to 3% Using Population II |
13694 |
Amanda R. Hendrix, Planetary Science Institute |
UV spectra of the icy Saturnian satellites: Understanding exogenic processes and NH3 in the system |
13695 |
Benne W. Holwerda, Sterrewacht Leiden |
STarlight Absorption Reduction through a Survey of Multiple Occulting Galaxies (STARSMOG) |
13700 |
Carl Melis, University of California - San Diego |
Confirming the most water-rich extrasolar rocky body |
13704 |
Steven G. Parsons, Universidad de Valparaiso |
Testing the single degenerate channel for supernova Ia |
13728 |
Steven Kraemer, Catholic University of America |
Do QSO2s have Narrow Line Region Outflows? Implications for quasar-mode feedback |
13741 |
Thaisa Storchi-Bergmann, Universidade Federal do Rio Grande do Sul |
Constraining the structure of the Narrow-Line Region of nearby QSO2s |
13750 |
John M. Cannon, Macalester College |
Fundamental Parameters of the SHIELD II Galaxies |
13760 |
Derck L. Massa, Space Science Institute |
Filling the gap --near UV, optical and near IR extinction |
13767 |
Michele Trenti, University of Melbourne |
Bright Galaxies at Hubble's Detection Frontier: The redshift z~9-10 BoRG pure-parallel survey |
13777 |
Michael D. Gregg, University of California - Davis |
Morphological Transformation in the Coma Cluster |
13784 |
Robert M. Quimby, San Diego State University |
The First UV Spectra of a Hydrogen-Rich Superluminous Supernova |
13793 |
Rebecca A A Bowler, Royal Observatory Edinburgh |
Unveiling the merger fraction, sizes and morphologies of the brightest z ~ 7 galaxies |
13804 |
Kristen McQuinn, University of Minnesota - Twin Cities |
Important Nearby Galaxies without Accurate Distances |
13821 |
Andrew C. Fabian, University of Cambridge |
H-alpha Filaments and Feedback in NGC4696 at the centre of the Centaurus cluster |
13826 |
Massimo Robberto, Space Telescope Science Institute |
The Orion Nebula Cluster as a Paradigm of Star Formation |
13833 |
Nicolas Tejos, University of California - Santa Cruz |
Characterizing the cool and warm-hot intergalactic medium in clusters at z < 0.4 |
14052 |
Michael C. Cushing, University of Toledo |
A Spitzer/HST Case Study of Weather on a Y Dwarf |