| Earlier reports | Convert Day of Year |
Daily Report #10701
Period Covered:
08:00 PM October 30, 2025 - 07:59 PM October 31, 2025
(DOY 304/0000z - 304/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 17307 | Kim-Vy Tran, Harvard University | A Legacy Library of 500 Strong Gravitational Lenses |
| 17310 | Michael Koss, Eureka Scientific Inc. | A Blue Gap Survey of Nearby Active Galaxies |
| 17474 | Justin Pierel, Space Telescope Science Institute | Pioneering Precision: Advancing Cosmology with the First Statistical Sample of Gravitationally Lensed Supernovae |
| 17526 | Peter Senchyna, Carnegie Institution of Washington | Mega-deep UV spectroscopy of star-forming galaxies: completing the picture of the extremely metal-poor massive stars underlying high-ionization UV nebular emission |
| 17757 | Sapna Mishra, Space Telescope Science Institute | Probing the front-side of the Circumgalactic Medium of the Large Magellanic Cloud |
| 17770 | Daichi Hiramatsu, University of Florida | Unveiling the Progenitors of Interacting Supernovae with Resolved Host Galaxy Imaging in the Rest-Frame UV |
| 17802 | Jeyhan Kartaltepe, Rochester Institute of Technology | CLUTCH: The COSMOS Legacy UV-Optical Treasury Campaign with Hubble |
| 17833 | Julianne Dalcanton, University of Washington | Bringing HST to the VLA: The Interaction of Stars and Gas in the Local Group |
| 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 |
| 17634 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Hot Pixel Annealing |
| 17655 | Alyssa Guzman, Space Telescope Science Institute | CCD Daily Monitor (Part 3) |
| 17666 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS Bowtie Monitor |
| 17669 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |