Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #10392

Period Covered:
07:00 PM December 25, 2024 - 06:59 PM December 26, 2024
(DOY 361/0000z - 361/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
17151 Matteo Messa, INAF - OAS Bologna Massive star clusters in low star formation regime dwarfs?
17526 Peter Senchyna, Carnegie Institution of Washington Mega-deep UV spectroscopy of star-forming galaxies: completing the picture of the extremely metal-poor massive stars underlying high-ionization UV nebular emission
17743 Adam Riess, The Johns Hopkins University Which dust is it? Unveiling Cosmic Mysteries by Redefining Dust and Distance in the Universe
17765 Matt Nicholl, Queen's University Belfast GHOSTBUSTERS: Determining the origin of tidal disruption events with a high-resolution survey of their host galaxies
17802 Jeyhan Kartaltepe, Rochester Institute of Technology CLUTCH: The COSMOS Legacy UV-Optical Treasury Campaign with Hubble
17892 Doyee Byun, University of Michigan A Coordinated UV and X-ray Reverberation Study of NGC 4151 at High Spectral Resolution
Calibration Observations Scheduled
17629 Matthew Dallas, Space Telescope Science Institute STIS CCD Dark Monitor Part 1
17632 Joshua Lothringer, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 1
17634 Matthew Dallas, Space Telescope Science Institute STIS CCD Hot Pixel Annealing
17647 Jacqueline Brown, Space Telescope Science Institute STIS MAMA FUV Flat-Field Monitor
17666 Aidan Pidgeon, Space Telescope Science Institute WFC3 UVIS Bowtie Monitor
17667 Aidan Pidgeon, Space Telescope Science Institute WFC3 UVIS CCD Daily Monitor Part 1
17670 Isabel Rivera, Space Telescope Science Institute WFC3 UVIS CCD Unflashed (CTE) Monitor
17852 Leonardo Dos Santos, Space Telescope Science Institute Cycle 32 COS FUV Split-Wavecal Calibration Program
17884 Debopam Som, Space Telescope Science Institute Verification of Target Placement for COS at LP7 and LP10