| Program |
Principal Investigator |
Program Title |
| Science Observations Scheduled |
| 12445 |
Sandra Faber, University of California - Santa Cruz |
Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey -- GOODS-North Field, Late Visits of SNe Search |
| 12472 |
Claus Leitherer, Space Telescope Science Institute |
CCC - The Cosmic Carbon Conundrum |
| 12486 |
David Bowen, Princeton University |
QSO Absorption Line Systems from Dwarf Galaxies |
| 12500 |
Sugata Kaviraj, University of Hertfordshire |
High-resolution UV studies of SAURON galaxies with WFC3: constraining recent star formation and its drivers in local early-type galaxies |
| 12568 |
Matthew Malkan, University of California - Los Angeles |
WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time |
| 12572 |
Michele Trenti, University of Cambridge |
The Brightest of Reionizing Galaxies Pure Parallel Survey |
| 12870 |
Boris Gaensicke, The University of Warwick |
The mass and temperature distribution of accreting white dwarfs |
| 12874 |
David Floyd, Monash University |
Quasar accretion disks: is the standard model valid? |
| 12880 |
Adam Riess, The Johns Hopkins University |
The Hubble Constant: Completing HST's Legacy with WFC3 |
| 12903 |
Luis Ho, Carnegie Institution of Washington |
The Evolutionary Link Between Type 2 and Type 1 Quasars |
| 13046 |
Robert Kirshner, Harvard University |
RAISIN: Tracers of cosmic expansion with SN IA in the IR |
| Calibration Observations Scheduled |
| 12803 |
Knox Long, Space Telescope Science Institute |
Guard Darks |
| 13074 |
John Biretta, Space Telescope Science Institute |
UVIS CCD Daily Monitor B |
| 13131 |
Svea Hernandez, Space Telescope Science Institute |
CCD Dark Monitor Part 1 |
| 13133 |
Svea Hernandez, Space Telescope Science Institute |
CCD Bias and Read Noise Monitor Part 1 |
| 13153 |
David Golimowski, Space Telescope Science Institute |
CCD Daily Monitor {Part 2} |
| 13162 |
Ralph Bohlin, Space Telescope Science Institute |
ACS Photometric Cross-Calibration using Stellar Flux Standards |