Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #10634

Period Covered:
08:00 PM August 24, 2025 - 07:59 PM August 25, 2025
(DOY 237/0000z - 237/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
17696 Kevin France, University of Colorado at Boulder Can NUV Flares Kickstart Prebiotic Chemical Chains on M Dwarf Planets?
17697 Matti Dorsch, Universitat Potsdam A far-UV treasury survey for hot subdwarf stars
17704 Andreas Sander, Astronomisches Rechen-Institut Heidelberg Mapping the iron abundances and winds of the OB population across the Magellanic Bridge
17749 Travis Fischer, Space Telescope Science Institute - ESA - JWST A UV IFU in Space: Observations of AGN Feedback and Star Formation in NGC 1068
17831 Moire Prescott, New Mexico State University Ionization Echoes of Fading AGN
17833 Julianne Dalcanton, University of Washington Bringing HST to the VLA: The Interaction of Stars and Gas in the Local Group
17843 Amy Simon, NASA Goddard Space Flight Center Hubble 2020: Outer Planet Atmospheres Legacy (OPAL) Program
Calibration Observations Scheduled
17616 Christian Johnson, Space Telescope Science Institute Cycle 32 COS NUV Detector Dark Monitor
17631 Matthew Dallas, Space Telescope Science Institute STIS CCD Dark Monitor Part 3
17633 Joshua Lothringer, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 2
17646 Jacqueline Brown, Space Telescope Science Institute STIS NUV MAMA Dark Monitor
17655 Alyssa Guzman, Space Telescope Science Institute CCD Daily Monitor (Part 3)
17669 Aidan Pidgeon, Space Telescope Science Institute WFC3 UVIS CCD Daily Monitor Part 3
17670 Isabel Rivera, Space Telescope Science Institute WFC3 UVIS CCD Unflashed (CTE) Monitor
17671 Catherine Martlin, Space Telescope Science Institute WFC3 UVIS Post-flash Monitor
17689 Frederick Dauphin, Space Telescope Science Institute WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats
17852 Leonardo Dos Santos, Space Telescope Science Institute Cycle 32 COS FUV Split-Wavecal Calibration Program