Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
15132 |
Harald Ebeling, University of Hawaii |
Beyond MACS: A Snapshot Survey of the Most Massive Clusters of Galaxies at z>0.5 |
15446 |
Julianne Dalcanton, University of Washington |
Establishing HST's Low Redshift Archive of Interacting Systems |
15628 |
Beth Biller, University of Edinburgh, Institute for Astronomy |
A search for sub-Jupiter mass companions to young planetary mass brown dwarfs |
15638 |
Denis Grodent, Universite de Liege |
Auroral and magnetospheric context for Juno in situ instruments during Cycle 26 |
15643 |
Matthew Hayes, Stockholm University |
The Cosmic Evolution of Circumgalactic Gas and Lyman alpha Halos |
15652 |
Tommaso Treu, University of California - Los Angeles |
H0, the stellar initial mass function, and other dark matters from a large sample of quadruply imaged quasars |
15654 |
Janice Lee, California Institute of Technology |
PHANGS-HST: Linking Stars and Gas throughout the Scales of Star Formation |
15656 |
Joshua Peek, Space Telescope Science Institute |
QuaStar: The first unobscured view of the Milky Way's Circumgalactic Medium |
15659 |
Douglas Gies, Georgia State University Research Foundation |
The Missing Link in Massive Binary Star Evolution |
Calibration Observations Scheduled |
15521 |
Tyler Desjardins, Space Telescope Science Institute |
CCD Daily Monitor (Part 3) |
15533 |
Camellia Magness, Space Telescope Science Institute |
COS/FUV Detector Dark Monitor |
15538 |
Camellia Magness, Space Telescope Science Institute |
COS/NUV Detector Dark Monitor |
15548 |
Doug Branton, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 3 |
15550 |
Doug Branton, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 2 |
15571 |
Catherine Martlin, Space Telescope Science Institute |
WFC3 UVIS Daily Monitor C |
15578 |
Ben Sunnquist, Space Telescope Science Institute |
IR Dark Monitor |
15589 |
Clare Shanahan, Space Telescope Science Institute |
WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |