Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #8879

Period Covered:
07:00 PM November 03, 2020 - 06:59 PM November 04, 2020
(DOY 309/0000z - 309/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
15864 Goetz Graefener, Universitat Bonn, Argelander Institute for Astronomy Is the Type Ic supernova progenitor WS35 a white dwarf merger product?
15879 Adam Riess, The Johns Hopkins University A Measurement of the Gaia Offset to Build a Superior Distance Ladder and Resolve the Origin of the Hubble Tension
15932 Martha Boyer, Space Telescope Science Institute Uncovering the Cause of the Shift in Carbon Star Behaviour at High Metallicity
16181 Laura Kreidberg, Max Planck Institute for Astronomy Exploring the Demographics of Exo-Neptunes: Atmospheric Characterization of a Cool Sub-Neptune from TESS
16183 Simon Porter, Southwest Research Institute Followup High-Precision Astrometry and Binary Searches of Potential New Horizons KBO Targets
16223 Marco Gullieuszik, Osservatorio Astronomico di Padova Star-forming clumps in jellyfish galaxy tails
16227 David Bowen, Princeton University Extremely Metal Poor Galaxies (XMPGs): A Search for the Lowest Metallicity Gas in Nearby Galaxies
16241 Michael Koss, Eureka Scientific Inc. A NUV Snapshot Survey of the Nearest Luminous AGN
16359 Hans Guenther, Massachusetts Institute of Technology A pure-parallel search for faint stuff in star forming regions
Calibration Observations Scheduled
15716 Catherine Martlin, Space Telescope Science Institute WFC3 UVIS CCD Daily Monitor Part 3
16337 Matthew Maclay, Space Telescope Science Institute STIS CCD Dark Monitor Part 1
16340 Matthew Maclay, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 1
16377 Meaghan McDonald, Space Telescope Science Institute CCD Daily Monitor (Part 1)
16402 Jennifer Medina, Space Telescope Science Institute WFC3 UVIS Traps with Charge Injection
16419 Jenna Ryon, Space Telescope Science Institute ACS/WFC Darks with Reduced Exposure Time and Post-Flash