| Earlier reports | Convert Day of Year |
Daily Report #10850
Period Covered:
08:00 PM March 28, 2026 - 07:59 PM March 29, 2026
(DOY 088/0000z - 088/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 17513 | Paul Bennet, Space Telescope Science Institute | Proper Motions of Galaxies in the M81 Group: Unleashing the Full Power of HST's 20-year Time Baseline |
| 17744 | Stephen Lawrence, Hofstra University | Reflections of a Violent Past: Using Light Echoes to Survey Historical Supernovae in M82 |
| 17776 | Sean Terry, University of Maryland | A Precursor Survey of the Roman Galactic Bulge Time Domain Fields |
| 17779 | Scott Chapman, University of British Columbia | A massive protocluster at z=4.3 selected by the South Pole Telescope |
| 17833 | Julianne Dalcanton, Flatiron Institute | Bringing HST to the VLA: The Interaction of Stars and Gas in the Local Group |
| 18025 | Davide Massari, INAF - Osservatorio di Astrofisica e Scienza dello Spazio | Last but not least: 13 globular clusters to complete the HST legacy |
| Calibration Observations Scheduled | ||
| 17936 | Jacqueline Hernandez, Space Telescope Science Institute | Cycle 33 COS NUV Spectroscopic Sensitivity Monitor |
| 17947 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 2 |
| 17949 | Isabel Rivera, Space Telescope Science Institute | WFC3 UVIS CCD Unflashed (CTE) Monitor |
| 17956 | Joel Green, Space Telescope Science Institute | WFC3 IR Dark Monitor |
| 17969 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |
| 18155 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
| 18157 | Joshua Lothringer, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
| 18197 | Christian Johnson, Space Telescope Science Institute | Cycle 33 FUV Detector Dark Monitor |
| 18221 | Daniel Stapleton, Space Telescope Science Institute | Supplemental NUV Sensitivity Monitoring Through Solar Maximum |