Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
15073 |
Boris Gaensicke, The University of Warwick |
Extreme evolved solar systems (EESS) |
15126 |
Danielle Berg, The Ohio State University |
Resolving the Abundance Discrepancy with HST/COS |
15133 |
Peter Erwin, Max-Planck-Institut fur extraterrestrische Physik |
Solving the Mystery of Galaxy Bulges and Bulge Substructure |
15182 |
David Sand, University of Arizona |
The Origin of Ultra-Faint Galaxies |
15211 |
Letizia Stanghellini, National Optical Astronomy Observatory, AURA |
Carbon in dusty, compact Galactic planetary nebulae: A study of AGB evolution and recycling in the Milky Way |
15212 |
Michele Trenti, University of Melbourne |
The brightest galaxies in the first 700 Myr: Building Hubble's legacy of large area IR imaging for JWST and beyond |
15266 |
Zheng Cai, University of California - Santa Cruz |
Imaging the Most Massive Galaxy Overdensities at z=2.2: The Morphology-Density Relation at High Redshift |
15678 |
Karen Meech, University of Hawaii |
Comet or break-up? The physical nature of Gault's dust trail |
Calibration Observations Scheduled |
15485 |
Ralph Bohlin, Space Telescope Science Institute |
CAL/STIS: Standard Stars for the JWST Mission and CALSPEC Legacy |
15519 |
Tyler Desjardins, Space Telescope Science Institute |
CCD Daily Monitor (Part 1) |
15524 |
Tyler Desjardins, Space Telescope Science Institute |
CCD Hot Pixel Annealing |
15546 |
Doug Branton, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 1 |
15549 |
Doug Branton, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 1 |
15568 |
Heather Kurtz, Space Telescope Science Institute |
UVIS Bowtie Monitor |
15569 |
Catherine Martlin, Space Telescope Science Institute |
WFC3 UVIS Daily Monitor A |
15573 |
Catherine Martlin, Space Telescope Science Institute |
UVIS Post-flash monitor |
15577 |
Jennifer Medina, Space Telescope Science Institute |
WFC3 Characterization of UVIS traps with CI |
15592 |
Ben Sunnquist, Space Telescope Science Institute |
WFC3 CSM monitor with earth flats |