| Earlier reports | Convert Day of Year |
Daily Report #10772
Period Covered:
07:00 PM January 09, 2026 - 06:59 PM January 10, 2026
(DOY 010/0000z - 010/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 16875 | George Dransfield, University of Oxford | Reconnaissance Transmission Spectroscopy of The BEST Temperate Mini-Neptune for Atmospheric Characterisationround |
| 17719 | Maximilien Franco, Universite Paris-Saclay | Brighter than GN-z11? Grism Observations of the brightest z~11 Candidates found in COSMOS-Web |
| 17729 | Nimisha Kumari, Space Telescope Science Institute - ESA - JWST | Decoding Reionization Era using UV and IR spectral features |
| 17775 | Charlotte Angus, Queen's University Belfast | Double Trouble: Understanding the Origins of Double Peaked Tidal Disruption Events |
| 17780 | John Noonan, Auburn University | Testing The Refractory Sulfur Reservoir Hypothesis with the Next Interstellar Object |
| 17802 | Jeyhan Kartaltepe, Rochester Institute of Technology | CLUTCH: The COSMOS Legacy UV-Optical Treasury Campaign with Hubble |
| 18103 | David Thilker, The Johns Hopkins University | Anatomy of a fall: Dissecting the environment-driven transformation of late-type Virgo cluster galaxies with HST UV-optical imaging of star clusters, associations, and HII regions |
| Calibration Observations Scheduled | ||
| 17693 | Catherine Martlin, Space Telescope Science Institute | WFC3 Astrometric Scale Monitoring |
| 17934 | Christian Johnson, Space Telescope Science Institute | Cycle 33 NUV Detector Dark Monitor |
| 17946 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 1 |
| 18154 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Dark Monitor Part 1 |
| 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 |
| 18199 | Jacqueline Hernandez, Space Telescope Science Institute | Cycle 33 COS FUV Spectroscopic Sensitivity Monitor |