Earlier reports | Convert Day of Year |
Daily Report #10667
Period Covered:
08:00 PM September 26, 2025 - 07:59 PM September 27, 2025
(DOY 270/0000z - 270/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
17474 | Justin Pierel, Space Telescope Science Institute | Pioneering Precision: Advancing Cosmology with the First Statistical Sample of Gravitationally Lensed Supernovae |
17697 | Matti Dorsch, Universitat Potsdam | A far-UV treasury survey for hot subdwarf stars |
17726 | Haakon Dahle, University of Oslo | Time delay cosmography with strong cluster lenses |
17733 | Yong Zheng, Rensselaer Polytechnic Institute | When Clouds Collide: Observing Gas Accretion onto the Milky Way's Disk |
17770 | Daichi Hiramatsu, University of Florida | Unveiling the Progenitors of Interacting Supernovae with Resolved Host Galaxy Imaging in the Rest-Frame UV |
17912 | Matthew Bayliss, University of Cincinnati Main Campus | Mapping Spatially Resolved Neutral H In Strongly Lensed Quasar Host Galaxies With Narrowband Lyman-alpha |
17916 | Tommaso Treu, University of California - Los Angeles | Dark matter, the Hubble tension, and the stellar IMF from HST imaging of quadruply imaged quasars |
Calibration Observations Scheduled | ||
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 |
17669 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
17671 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS Post-flash Monitor |
17685 | Linda Dressel, Space Telescope Science Institute | HST Cycle 32 Focus & Optical Monitor |
17692 | Frederick Dauphin, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
17850 | Christian Johnson, Space Telescope Science Institute | Cycle 32 FUV Detector Dark Monitor |
17888 | Daniel Stapleton, Space Telescope Science Institute | Supplemental NUV Sensitivity Monitoring Through Solar Maximum |
17906 | Annalisa Calamida, Space Telescope Science Institute | HST/WFC3 Observations for Cross-Mission Flux Calibration |