Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #9619

Period Covered:
07:00 PM November 13, 2022 - 06:59 PM November 14, 2022
(DOY 318/0000z - 318/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
15445 William Keel, University of Alabama Gems of the Galaxy Zoos
16233 Christian Schneider, Universitat Hamburg, Hamburger Sternwarte Jets and disk scattering - Spatially resolved optical and FUV observations of AA Taudac
16659 Anna Pala, ESA-European Space Astronomy Centre Accreting white dwarfs as probes of compact binary evolution
16672 Yuri Izotov, Ukrainian National Academy of Sciences, BITP Ly-alpha emission from the low-z most metal-deficient star-forming galaxies
16705 Doron Chelouche, University of Haifa Shedding light on light echoes: mapping the accretion disk and broad line region in Mrk 279
16786 Claire Murray, Space Telescope Science Institute Scylla: a pure-parallel, multi-headed attack on dust evolution and star formation in ULLYSES galaxies
16820 Julia Roman-Duval, Space Telescope Science Institute ULLYSES LMC O5-O6 Dwarfs - STIS
17098 Adam Riess, The Johns Hopkins University HST and Gaia, with Light and Distances, a Foundational Legacy of the Distance Ladder
17112 Nicole Reindl, Universitat Potsdam A Treasury FUV Survey of the Hottest White Dwarfs
17225 Daniela Calzetti, University of Massachusetts - Amherst The (Ir)Regularities of Dust Attenuation in Star Forming Galaxies
Calibration Observations Scheduled
16568 Benjamin Kuhn, Space Telescope Science Institute WFC3 UVIS CCD Daily Monitor Part 3
16946 Sophia Medallon, Space Telescope Science Institute STIS CCD Dark Monitor Part 1
16949 Doug Branton, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 1
16970 Meaghan McDonald, Space Telescope Science Institute CCD Daily Monitor (Part 1)
17011 Frederick Dauphin, Space Telescope Science Institute WFC3 IR Dark Monitor
17019 Benjamin Kuhn, Space Telescope Science Institute WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats