Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
17069 |
Matthew Hayes, Stockholm University |
The Lyman-alpha and Continuum Origins Survey (LaCOS) |
17110 |
David Setton, Princeton University |
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 |
17172 |
Rebecca Canning, University of Portsmouth |
Caught in the act: Galaxy quenching beyond the core of a redshift two galaxy cluster? |
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 |
17181 |
Joseph Lyman, The University of Warwick |
A public survey of superluminous supernovae hosts to study their progenitors |
17185 |
Laura Rogers, University of Cambridge |
How diverse is the bulk composition of exoplanetary material? |
17309 |
Vihang Mehta, California Institute of Technology |
Resolved imaging survey of the analogs of high-z massive, star-forming clumps |
17434 |
Eduardo Vitral, Space Telescope Science Institute |
Shedding Light on Dark Matter: Internal Proper Motions in Ursa Minor |
Calibration Observations Scheduled |
17005 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 3 |
17324 |
Christian Johnson, Space Telescope Science Institute |
Cycle 31 FUV Detector Dark Monitor |
17357 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 IR Dark Monitor |
17361 |
Annalisa Calamida, Space Telescope Science Institute |
WFC3 UVIS and IR Photometry |
17368 |
Benjamin Kuhn, Space Telescope Science Institute |
WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |
17371 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |
17374 |
Sophia Medallon, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 1 |
17377 |
Daniel Stapleton, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 1 |