| Program |
Principal Investigator |
Program Title |
| Science Observations Scheduled |
| 17100 |
Yuri Izotov, Ukrainian National Academy of Sciences, BITP |
UV spectra of the most metal-deficient galaxies |
| 17110 |
David Setton, University of Pittsburgh |
Post-starbursts from DESI: Timing quenching and morphological transformation at 1 < z < 1.3 |
| 17115 |
David Bowen, Princeton University |
The Circumgalactic Medium of Dwarf Galaxy Pairs |
| 17128 |
Ryan Foley, University of California - Santa Cruz |
Reducing Type Ia Supernova Distance Biases by Separating Reddening and Intrinsic Color |
| 17147 |
Claudia Scarlata, University of Minnesota - Twin Cities |
The Parallel Ionizing Emissivity Survey |
| 17211 |
Rongmon Bordoloi, North Carolina State University |
Search for feedback signatures in massive blue galaxy halos |
| 17227 |
Todd Tripp, University of Massachusetts - Amherst |
Unique Constraints on the Physics of Circumgalactic Gas from Ultrahigh Resolution Observations of Galactic High-Velocity Clouds |
| 17269 |
Xin Liu, University of Illinois at Urbana - Champaign |
A Complete Census of Luminous Sub-arcsec Dual/Lensed Quasars at z > 1.5 |
| 17308 |
Cameron Lemon, Ecole Polytechnique Federale de Lausanne |
An HST Gap Program for lensed Quasars |
| 17310 |
Michael Koss, Eureka Scientific Inc. |
A Blue Gap Survey of Nearby Active Galaxies |
| 17472 |
Andrew Levan, Radboud Universiteit Nijmegen |
Gamma-ray burst supernovae across cosmic time |
| Calibration Observations Scheduled |
| 16948 |
Sophia Medallon, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 3 |
| 16950 |
Sean Lockwood, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 2 |
| 16951 |
Sophia Medallon, Space Telescope Science Institute |
STIS CCD Hot Pixel Annealing |
| 17005 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 3 |
| 17006 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Unflashed (CTE) Monitor |
| 17022 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |