| Program |
Principal Investigator |
Program Title |
| Science Observations Scheduled |
| 15445 |
William Keel, University of Alabama |
Gems of the Galaxy Zoos |
| 16716 |
Kailash Sahu, Space Telescope Science Institute |
Snapshot Survey of Historical Microlensing Events |
| 16813 |
Julia Roman-Duval, Space Telescope Science Institute |
ULLYSES LMC O3 Supergiants - COS |
| 16928 |
RL Beaton, Princeton University |
Securing the Absolute Scale for the IR-TRGB Distance Ladder |
| 17108 |
Justin Spilker, Texas A & M University |
Dissecting Early Universe Dust with Matched-Resolution Observations from HST, JWST, and ALMA |
| 17198 |
Peter Senchyna, Carnegie Institution of Washington |
First look at the high-ionization UV nebular emission powered by the youngest stellar populations below 5% solar metallicity: the missing link to the reionization era? |
| 17201 |
Eileen Meyer, University of Maryland Baltimore County |
Determining the High-Energy Emission Mechanism in Extragalactic Jets with HST |
| 17216 |
Alessandro Savino, University of California - Berkeley |
Establishing a 1% anchor for the Population II Distance Ladder with HST and Gaia |
| 17298 |
Eleonora Troja, Universita di Roma Tor Vergata |
The afterglow, supernova and distance scale of a record-breaking gamma-ray burst |
| Calibration Observations Scheduled |
| 16947 |
Sophia Medallon, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 2 |
| 16949 |
Sean Lockwood, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 1 |
| 16951 |
Sophia Medallon, Space Telescope Science Institute |
STIS CCD Hot Pixel Annealing |
| 17004 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 2 |
| 17006 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Unflashed (CTE) Monitor |
| 17019 |
Benjamin Kuhn, Space Telescope Science Institute |
WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |
| 17022 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |