| Program |
Principal Investigator |
Program Title |
| Science Observations Scheduled |
| 15444 |
Aaron Barth, University of California - Irvine |
An ACS Schedule Gap Imaging Survey of Nearby Active Galaxies |
| 16990 |
Tuan Do, University of California - Los Angeles |
Advancing a decades long experiment at the Galactic center |
| 17097 |
Adam Riess, The Johns Hopkins University |
Reinforcing the Distance Ladder with Cepheids in the Core of the SMC |
| 17104 |
Matthew Rickard, University College London |
Repeated Stellar Wind Line Variability in O Stars in the SMC |
| 17167 |
Herve Bouy, Universite de Bordeaux |
Multiplicity among free-floating planets |
| 17185 |
Laura Rogers, University of Cambridge |
How diverse is the bulk composition of exoplanetary material? |
| 17396 |
Antonio Martin-Carrillo, University College Dublin |
Revealing the progenitor of the dirty fireball gamma-ray burst AT 2023lcr through its supernova component |
| 17397 |
Subo Dong, Peking University |
Confirming the first isolated dark stellar remnant candidate discovered by interferometric microlensing |
| 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 |
| 16972 |
Meaghan McDonald, Space Telescope Science Institute |
CCD Daily Monitor (Part 3) |
| 17005 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 3 |
| 17022 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |
| 17247 |
Christian Johnson, Space Telescope Science Institute |
Cycle 30 FUV Detector Dark Monitor |
| 17260 |
Varun Bajaj, Space Telescope Science Institute |
WFC3 IR Time-Dependent Sensitivity: Clusters |
| Other Observations Scheduled |
| 15601 |
David Sahnow, Space Telescope Science Institute |
COS FUV DCE Memory Dump |
| 15962 |
Merle Reinhart, Space Telescope Science Institute |
Routine EEPROM dumps for ACS, COS, STIS, and WFC3 |