| Earlier reports | Convert Day of Year |
Daily Report #10621
Period Covered:
08:00 PM August 11, 2025 - 07:59 PM August 12, 2025
(DOY 224/0000z - 224/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 16747 | Karl Misselt, University of Arizona | FUV-Optical Spectroscopic Mapping of the PDRs in NGC7023 and The Horsehead |
| 17308 | Cameron Lemon, Stockholm University | An HST Gap Program for lensed Quasars |
| 17436 | Joseph Jensen, Utah Valley University | An Independent High-Precision Distance Ladder for Cosmology |
| 17756 | Paul Goudfrooij, Space Telescope Science Institute | Quantifying the Link Between the UV Upturn in Elliptical Galaxies and Multiple Stellar Populations In Globular Clusters |
| 17764 | Kyra Bostroem, University of Arizona | Unraveling Red Supergiant Mass Loss with Early FUV Spectra of a Type IIP/L Supernova |
| 17774 | Joseph Burchett, New Mexico State University | Multiphase gas in eROSITA-detected galaxy groups and clusters |
| 17847 | Jillian Rastinejad, University of Maryland | Identifying a New Source of r-Process Nucleosynthesis with HST |
| Calibration Observations Scheduled | ||
| 17616 | Christian Johnson, Space Telescope Science Institute | Cycle 32 COS NUV Detector Dark Monitor |
| 17631 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Dark Monitor Part 3 |
| 17633 | Joshua Lothringer, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
| 17635 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Spectroscopic Flats |
| 17641 | Daniel Stapleton, Space Telescope Science Institute | STIS/CCD Spectroscopic Sensitivity Monitor |
| 17669 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
| 17670 | Isabel Rivera, Space Telescope Science Institute | WFC3 UVIS CCD Unflashed (CTE) Monitor |
| 17692 | Frederick Dauphin, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
| 17852 | Leonardo Dos Santos, Space Telescope Science Institute | Cycle 32 COS FUV Split-Wavecal Calibration Program |