| Earlier reports | Convert Day of Year |
Daily Report #9163
Period Covered:
08:00 PM August 14, 2021 - 07:59 PM August 15, 2021
(DOY 227/0000z - 227/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 15446 | Julianne Dalcanton, University of Washington | Establishing HST's Low Redshift Archive of Interacting Systems |
| 16110 | Julia Roman-Duval, Space Telescope Science Institute | ULLYSES Monitoring Observations of the T Tauri Star RU Lup: First Epoch |
| 16196 | Gerard Kriss, Space Telescope Science Institute | Mapping Gas Flows in AGNs by Reverberation |
| 16205 | John Wisniewski, University of Oklahoma Norman Campus | Time Domain Coronagraphy: Diagnosing the Stripping of AU Mic's Debris Disk |
| 16229 | Clemence Fontanive, University of Bern | Precise distances and photometry for the Y dwarf population: unlocking the secrets of our coolest neighbours |
| 16230 | Derck Massa, Space Science Institute | An NUV SNAP program to supplement and enhance the value of the ULLYSES OB star legacy data. |
| 16239 | Ryan Foley, University of California - Santa Cruz | Snapshot Observations of Nearby, Recent Supernovae and Their Environments |
| 16280 | Mario De Pra, University of Central Florida Board of Trustees | Quasi-Hildas Objects: The Missing Link Between The Hildas and Centaurs Populations |
| Calibration Observations Scheduled | ||
| 16324 | Kate Rowlands, Space Telescope Science Institute | Cycle 28 COS FUV Spectroscopic Sensitivity Monitor |
| 16339 | Doug Branton, Space Telescope Science Institute | STIS CCD Dark Monitor Part 3 |
| 16341 | Doug Branton, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
| 16393 | Harish Khandrika, Space Telescope Science Institute | UVIS Bowtie Monitor |
| 16396 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
| 16412 | Jennifer Medina, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
| 16416 | Annalisa Calamida, Space Telescope Science Institute | WFC3 UVIS Time Dependent Sensitivity |