| Earlier reports | Convert Day of Year |
Daily Report #10901
Period Covered:
08:00 PM May 18, 2026 - 07:59 PM May 19, 2026
(DOY 139/0000z - 139/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 17833 | Julianne Dalcanton, Flatiron Institute | Bringing HST to the VLA: The Interaction of Stars and Gas in the Local Group |
| 18008 | Charles Kilpatrick, Northwestern University | Using HST to Find Supernova Progenitor Stars in JWST, HST, and Euclid Imaging |
| 18049 | Erica Hammerstein, University of California - Berkeley | Multi-Epoch UV Spectroscopy of Young Tidal Disruption Events |
| 18056 | David Rupke, Rhodes College | Growing in the Wind: OVI Spectroscopy of Cool Clouds mixing with a Hot CGM |
| 18060 | Antoine Bedard, University of Warwick | Opening the crucial ultraviolet window on carbon dredge-up in white dwarfs |
| 18095 | Sean Linden, Rochester Institute of Technology | The Hidden Engines That Could: Tracing Clump Formation and Evolution in the Hearts of Infrared-Luminous AGN Hosts |
| 18097 | Tian Li, Portsmouth University/ICG | Breaking the mass sheet degeneracy in strong lensing time delay cosmology with a new sample of double source plane lenses. |
| 18098 | Amy Bonsor, University of Cambridge | Is Sulfur stored in the refractory or volatile component of planetary building blocks? |
| Calibration Observations Scheduled | ||
| 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 |
| 17972 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
| 18155 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
| 18158 | Joshua Lothringer, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
| 18202 | Leonardo Dos Santos, Space Telescope Science Institute | Cycle 33 COS FUV Split-Wavecal Calibration Program |
| 18204 | Jacqueline Hernandez, Space Telescope Science Institute | Cycle 33 COS FUV Change in Spectroscopic Sensitivity Trends |