Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #8876

Period Covered:
08:00 PM October 31, 2020 - 06:59 PM November 01, 2020
(DOY 306/0000z - 306/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
15932 Martha Boyer, Space Telescope Science Institute Uncovering the Cause of the Shift in Carbon Star Behaviour at High Metallicity
15944 Trent Dupuy, University of Edinburgh, Institute for Astronomy The Coolest Sample of Brown Dwarf Dynamical Masses
16183 Simon Porter, Southwest Research Institute Followup High-Precision Astrometry and Binary Searches of Potential New Horizons KBO Targets
16195 Jonathan Nichols, University of Leicester A Tail of Two Giants: Observing Saturn's FUV auroras in Jupiter's magnetotail in 2020
16241 Michael Koss, Eureka Scientific Inc. A NUV Snapshot Survey of the Nearest Luminous AGN
16243 Federico Marocco, California Institute of Technology Determining the low-mass cutoff for star formation
16257 Francine Marleau, Universitat Innsbruck, Institut fur Astronomie Globular cluster systems of ultra-diffuse galaxies in low density environments
16261 Sally Oey, University of Michigan Mrk 71: Prototype for Catastrophic Cooling in a Green Pea Analog
16318 Gabor Worseck, Universitat Potsdam The First Measurement of the Distribution of Quasar Lifetimes with the HeII Proximity Effect
Calibration Observations Scheduled
15716 Catherine Martlin, Space Telescope Science Institute WFC3 UVIS CCD Daily Monitor Part 3
15737 Matthew Maclay, Space Telescope Science Institute STIS CCD Dark Monitor Part 3
15739 Matthew Maclay, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 2
16352 Joleen Carlberg, Space Telescope Science Institute MAMA Spectroscopic Sensitivity and Focus Monitor
16412 Jennifer Medina, Space Telescope Science Institute WFC3 CSM Monitor with Earth Flats
16415 Annalisa Calamida, Space Telescope Science Institute WFC3 UVIS and IR Photometry
16419 Jenna Ryon, Space Telescope Science Institute ACS/WFC Darks with Reduced Exposure Time and Post-Flash