Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #10297

Period Covered:
08:00 PM September 21, 2024 - 07:59 PM September 22, 2024
(DOY 266/0000z - 266/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
17098 Adam Riess, The Johns Hopkins University HST and Gaia, with Light and Distances, a Foundational Legacy of the Distance Ladder
17110 David Setton, Princeton University Post-starbursts from DESI: Timing quenching and morphological transformation at 1 < z < 1.3
17424 Rui Marques-Chaves, University of Geneva, Department of Astronomy High-resolution imaging of the ionizing and non-ionizing radiation of extreme starbursts at z~2.4
17442 Susana Deustua, National Institute of Standards and Technology Calibrating the Universe: Faint White Dwarf Standard Stars at the Ecliptic Poles for Cross-calibration of HST, Euclid and Roman.apt
17511 Jaya Maithil, Smithsonian Institution Astrophysical Observatory A Major Overhaul of Ultraviolet-Based Black Hole Mass Prescriptions
17518 Alexander Beckett, Space Telescope Science Institute PIE+: Identifying LyC leakers through improved photometry of the PIE survey fields
Calibration Observations Scheduled
17349 Aidan Pidgeon, Space Telescope Science Institute WFC3 UVIS CCD Daily Monitor Part 3
17350 Isabel Rivera, Space Telescope Science Institute WFC3 UVIS CCD Unflashed (CTE) Monitor
17351 Catherine Martlin, Space Telescope Science Institute WFC3 UVIS Post-flash Monitor
17362 Mariarosa Marinelli, Space Telescope Science Institute WFC3 UVIS Time Dependent Sensitivity
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
17376 Daniel Welty, Space Telescope Science Institute STIS CCD Dark Monitor Part 3
17378 Daniel Stapleton, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 2
17584 Daniel Stapleton, Space Telescope Science Institute Supplemental NUV Sensitivity Monitoring Through Solar Maximum