| Earlier reports | Convert Day of Year |
Daily Report #8981
Period Covered:
07:00 PM February 13, 2021 - 06:59 PM February 14, 2021
(DOY 045/0000z - 045/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 15445 | William Keel, University of Alabama | Gems of the Galaxy Zoos |
| 16056 | Keith Noll, NASA Goddard Space Flight Center | Recovery and Orbit of a Satellite of the Trojan Asteroid Eurybates - a Lucy Mission Target |
| 16187 | Feige Wang, University of Arizona | Mapping A Distant Protocluster Anchored by A Luminous Quasar in the Epoch of Reionization |
| 16196 | Bradley Peterson, The Ohio State University | Mapping Gas Flows in AGNs by Reverberation |
| 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 |
| 16288 | Smita Mathur, The Ohio State University | What governs the physics of the warm-hot circumgalactic medium? |
| 16289 | Antonino Milone, Universita degli Studi di Padova | Multiple stellar populations in Globular Clusters: exploring the low mass regime |
| 16302 | Ya-Lin Wu, National Taiwan Normal University | Accretion Rates as a Diagnostic Tool for the Origin of Planetary-mass Companions |
| 16316 | Elena Sabbi, Space Telescope Science Institute | GULP: Galaxy UV Legacy Project |
| Calibration Observations Scheduled | ||
| 16327 | Dzhuliya "Julia" Dashtamirova, Space Telescope Science Institute | Cycle 28 COS/NUV Detector Dark Monitor |
| 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 |
| 16394 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 1 |
| 16412 | Jennifer Medina, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
| 16438 | Joleen Carlberg, Space Telescope Science Institute | STIS MAMA Exploration of FUV Flux Variations at Off-Nominal Detector Positions |