Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
15078 |
Soeren Larsen, Radboud Universiteit Nijmegen |
Initial conditions of multiple populations in the dynamically most pristine globular cluster, NGC 2419 |
15113 |
Abhijit Saha, National Optical Astronomy Observatory, AURA |
Extending the DA white dwarf spectrophotometric network to the Southern Hemisphere |
15115 |
John Silverman, University of Tokyo |
Emergence of the supermassive black hole - galaxy mass relations at z > 1 |
15150 |
R. Tully, University of Hawaii |
Local Void Reflex: IR TRGB Distances to Obscured Galaxies at the South Supergalactic Pole |
15155 |
Siyi Xu, Gemini Observatory, Northern Operations |
Actively Disintegrating Astroids around a White Dwarf |
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 |
15215 |
Vardha Bennert, Cal Poly Corporation, Sponsored Programs Department |
A Local Baseline of the Black Hole Mass - Host Galaxy Scaling Relations for Active Galaxies |
15260 |
Jonathan Trump, University of Connecticut |
Ultraviolet Echoes of Quasar Accretion Disks |
Calibration Observations Scheduled |
14940 |
Mees Fix, Space Telescope Science Institute |
FUV Detector Dark Monitor |
14942 |
Mees Fix, Space Telescope Science Institute |
NUV Detector Dark Monitor |
14943 |
Thomas Wheeler, Space Telescope Science Institute |
COS NUV MAMA Fold Distribution |
14960 |
Allyssa Riley, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 2 |
14962 |
Allyssa Riley, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 1 |
14976 |
Thomas Wheeler, Space Telescope Science Institute |
STIS MAMA Fold Distribution |
14981 |
Catherine Martlin, Space Telescope Science Institute |
WFC3 UVIS Daily Monitor B |
14989 |
Julia Fowler, Space Telescope Science Institute |
UVIS CTI Monitor (EPER) |
14996 |
Myles Mckay, Space Telescope Science Institute |
WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats Monitor |