| Program |
Principal Investigator |
Program Title |
| Science Observations Scheduled |
| 17309 |
Vihang Mehta, California Institute of Technology |
Resolved imaging survey of the analogs of high-z massive, star-forming clumps |
| 17410 |
Ryan Foley, University of California - Santa Cruz |
Reducing Type Ia Supernova Distance Biases by Separating Reddening and Intrinsic Color |
| 17598 |
Pieter van Dokkum, Yale University |
The globular clusters of Dragonfly 44 |
| 17708 |
Yue Shen, University of Illinois at Urbana - Champaign |
The Black Hole Mass - Stellar Mass Relation with Reverberation Mapping AGNs at 1
|
| 17735 |
Adam Bolton, Stanford University |
Confirming Spectroscopic Strong Lens Candidates from the DESI One-Percent Survey |
| 17780 |
John Noonan, Auburn University |
Testing The Refractory Sulfur Reservoir Hypothesis with the Next Interstellar Object |
| 17796 |
Stefano Valenti, University of California - Davis |
Tracing the mass-loss history from type II supernova explosions back through the red supergaint phase. |
| 18055 |
Michael Wong, University of California - Berkeley |
Simultaneous mapping of ammonia on Jupiter with Juno and HST/WFC3 |
| 18085 |
Xiaosheng Huang, University of San Francisco |
Confirming Spectroscopic Strong Lenses Found in New Discovery Windows from DESI DR1 |
| Calibration Observations Scheduled |
| 17692 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |
| 17946 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 1 |
| 17950 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS Post-flash Monitor |
| 17951 |
Ky Huynh, Space Telescope Science Institute |
WFC3 UVIS CCD Gain Stability |
| 17960 |
Jennifer Mack, Space Telescope Science Institute |
WFC3 UVIS Photometry |
| 18154 |
Matthew Dallas, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 1 |
| 18157 |
Joshua Lothringer, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 1 |
| 18202 |
Leonardo Dos Santos, Space Telescope Science Institute |
Cycle 33 COS FUV Split-Wavecal Calibration Program |