| Earlier reports | Convert Day of Year |
Daily Report #9180
Period Covered:
08:00 PM August 31, 2021 - 07:59 PM September 01, 2021
(DOY 244/0000z - 244/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 15839 | Odette Toloza Castillo, Universidad Tecnica Federico Santa Maria | Mapping the distribution of the planetary debris accreted across the surface of the white dwarf G29-38 |
| 16107 | Julia Roman-Duval, Space Telescope Science Institute | ULLYSES Monitoring Observations of the T Tauri Star BP Tau: First Epoch |
| 16173 | Grant Tremblay, Smithsonian Institution Astrophysical Observatory | Hyperfine Temporal & Spatial Resolution of Stellar Ages amid Quasar-Driven gas flows: Unifying HST with MUSE and ALMA |
| 16175 | Aida Wofford, Universidad Nacional Autonoma de Mexico, Obs. Astron. Nac. | Can Very Massive Stars form at the low-metallicity threshold of the nearby Universe? |
| 16193 | Bertrand Bonfond, Universite de Liege | Building connections: Juno and STIS contemporaneous observations of Jupiter's magnetosphere and auroras |
| 16230 | Derck Massa, Space Science Institute | An NUV SNAP program to supplement and enhance the value of the ULLYSES OB star legacy data. |
| Calibration Observations Scheduled | ||
| 16336 | Doug Branton, Space Telescope Science Institute | STIS CCD Performance 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 |
| 16379 | Meaghan McDonald, Space Telescope Science Institute | CCD Daily Monitor (Part 3) |
| 16396 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
| 16400 | Harish Khandrika, Space Telescope Science Institute | WFC3 UVIS CTI Monitor (EPER) |
| 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 |