| Earlier reports | Convert Day of Year |
Daily Report #9087
Period Covered:
08:00 PM May 30, 2021 - 07:59 PM May 31, 2021
(DOY 151/0000z - 151/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 16183 | Simon Porter, Southwest Research Institute | Followup High-Precision Astrometry and Binary Searches of Potential New Horizons KBO Targets |
| 16196 | Gerard Kriss, Space Telescope Science Institute | Mapping Gas Flows in AGNs by Reverberation |
| 16269 | David Jones, University of California - Santa Cruz | Tension at the Breaking Point: Uncovering New Physics Through a Two-Rung Distance Ladder Measurement of the Hubble Constant |
| 16281 | Marco Chiaberge, Space Telescope Science Institute - ESA | High-redshift 3CR: witnessing the formation of the most massive galaxies, clusters and AGN in the Bright Ages |
| 16298 | Mattia Libralato, Space Telescope Science Institute - ESA - JWST | Enhancing the astrometric legacy of HST for globular clusters |
| 16478 | Julia Roman-Duval, Space Telescope Science Institute | ULLYSES Two M5 T Tauri Survey Stars in Cha I |
| Calibration Observations Scheduled | ||
| 16322 | Dzhuliya "Julia" Dashtamirova, Space Telescope Science Institute | Cycle 28 COS FUV Detector Dark Monitor |
| 16327 | Dzhuliya "Julia" Dashtamirova, Space Telescope Science Institute | Cycle 28 COS/NUV Detector Dark Monitor |
| 16338 | Matthew Maclay, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
| 16341 | Matthew Maclay, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
| 16342 | Matthew Maclay, Space Telescope Science Institute | STIS CCD Hot Pixel Annealing |
| 16378 | Meaghan McDonald, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
| 16381 | Jenna Ryon, Space Telescope Science Institute | ACS Internal CTE Monitor |
| 16395 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 2 |
| 16409 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |