Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #9367

Period Covered:
07:00 PM March 06, 2022 - 06:59 PM March 07, 2022
(DOY 066/0000z - 066/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
16256 Graham Harper, University of Colorado at Boulder A Sensitive Test for Far Ultraviolet CO absorption in the Outflow of our Nearest Supernova Progenitor - Antares
16486 Koji Mukai, NASA Goddard Space Flight Center The Symbiotic Recurrent Nova T CrB as it Approaches its Next Eruption
16642 Boris Gaensicke, The University of Warwick A legacy survey for evolved planetary systems within 100pc
16662 Nicholas Seymour, Curtin University Lyman-alpha Observations of a z=8.45 Powerful Radio Galaxy
16677 Daniel Stark, University of Arizona Massive Stellar Populations at Reionization Metallicities: Anchoring Stellar Population Models for the JWST Era
16679 Jessica Werk, University of Washington Mainly on the Plane: Solving the Milky Way CGM Anomaly with Low-Galactic-Latitude QSOs
16794 Eilat Glikman, Middlebury College Constraining the Physical Properties of a Candidate Dual QSO at Cosmic Noon
Calibration Observations Scheduled
16523 Meaghan McDonald, Space Telescope Science Institute CCD Daily Monitor (Part 2)
16535 Dzhuliya "Julia" Dashtamirova, Space Telescope Science Institute Cycle 29 COS/NUV Detector Dark Monitor
16545 Doug Branton, Space Telescope Science Institute STIS CCD Dark Monitor Part 2
16547 Doug Branton, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 1
16566 Benjamin Kuhn, Space Telescope Science Institute WFC3 UVIS CCD Daily Monitor Part 1
16569 Aidan Pidgeon, Space Telescope Science Institute WFC3 UVIS CCD Unflashed (CTE) Monitor
16584 Catherine Martlin, Space Telescope Science Institute WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats
16828 Dzhuliya "Julia" Dashtamirova, Space Telescope Science Institute Cycle 29 COS FUV Detector Dark Monitor
16908 William Fischer, Space Telescope Science Institute COS FUV LP6 Calibration: Dispersion Solutions