Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #8359

Period Covered:
08:00 PM June 02, 2019 - 07:59 PM June 03, 2019
(DOY 154/0000z - 154/2359z)

Program Principal Investigator Program Title
Science Observations Scheduled
15304 Julien de Wit, Massachusetts Institute of Technology Collecting the Puzzle Pieces: Completing HST's UV+NIR Survey of the TRAPPIST-1 System ahead of JWST
15307 Michael Gladders, University of Chicago Building the SPT-HST Legacy: Imaging Massive Clusters to z=1.5
15626 Anne Jaskot, Williams College The Low-Redshift Lyman Continuum Survey
15648 Alex Parker, Southwest Research Institute The Solar System Origins Legacy Survey
15652 Tommaso Treu, University of California - Los Angeles H0, the stellar initial mass function, and other dark matters from a large sample of quadruply imaged quasars
15661 Michael McDonald, Massachusetts Institute of Technology Testing the Limits of AGN Feedback in Starburst and QSO Central Cluster Galaxies
Calibration Observations Scheduled
15520 Tyler Desjardins, Space Telescope Science Institute CCD Daily Monitor (Part 2)
15523 Jenna Ryon, Space Telescope Science Institute ACS Internal CTE Monitor
15527 Samantha Hoffmann, Space Telescope Science Institute ACS Internal Flat Fields
15533 Camellia Magness, Space Telescope Science Institute COS/FUV Detector Dark Monitor
15538 Camellia Magness, Space Telescope Science Institute COS/NUV Detector Dark Monitor
15547 Doug Branton, Space Telescope Science Institute STIS CCD Dark Monitor Part 2
15550 Doug Branton, Space Telescope Science Institute STIS CCD Bias and Read Noise Monitor Part 2
15568 Heather Kurtz, Space Telescope Science Institute UVIS Bowtie Monitor
15570 Catherine Martlin, Space Telescope Science Institute WFC3 UVIS Daily Monitor B
15574 Julia Fowler, Space Telescope Science Institute WFC3 UVIS CCD Gain Stability
15578 Ben Sunnquist, Space Telescope Science Institute IR Dark Monitor
15589 Clare Shanahan, Space Telescope Science Institute WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats