| Program |
Principal Investigator |
Program Title |
| Science Observations Scheduled |
| 17076 |
Trystyn Berg, University of Milano-Bicocca |
The C IV in L* galaxies (CIViL*) survey -- Pinpointing the physical conditions and evolutionary stages of gaseous halos |
| 17099 |
Lorenz Roth, Royal Institute of Technology |
Ganymede's water atmosphere in eclipse |
| 17110 |
David Setton, University of Pittsburgh |
Post-starbursts from DESI: Timing quenching and morphological transformation at 1 < z < 1.3 |
| 17128 |
Ryan Foley, University of California - Santa Cruz |
Reducing Type Ia Supernova Distance Biases by Separating Reddening and Intrinsic Color |
| 17179 |
Lluis Galbany, Institute of Space Sciences (CSIC-IEEC) |
A public HST-UV snapshot survey of type Ia supernova host galaxies with pre-existing optical integral-field spectroscopy |
| 17241 |
Eileen Meyer, University of Maryland Baltimore County |
Examining the Variability of High-Redshift Jets |
| 17278 |
Ryan Chornock, University of California - Berkeley |
Testing the Limit: Late-time HST Observations of the Most Energetic GRB Ever |
| Calibration Observations Scheduled |
| 16945 |
Sean Lockwood, Space Telescope Science Institute |
STIS CCD Performance Monitor |
| 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 |
| 17002 |
Harish Khandrika, Space Telescope Science Institute |
WFC3 UVIS Bowtie Monitor |
| 17005 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 3 |
| 17008 |
Harish Khandrika, Space Telescope Science Institute |
WFC3 UVIS CTI Monitor (EPER) |
| 17010 |
Mariarosa Marinelli, Space Telescope Science Institute |
WFC3 Characterization of UVIS Traps with Charge Injection |
| 17247 |
Christian Johnson, Space Telescope Science Institute |
Cycle 30 FUV Detector Dark Monitor |
| 17251 |
Kate Rowlands, Space Telescope Science Institute - ESA - JWST |
Cycle 30 COS FUV Change in Spectroscopic Sensitivity Trends |