| Earlier reports | Convert Day of Year |
Daily Report #10417
Period Covered:
07:00 PM January 19, 2025 - 06:59 PM January 20, 2025
(DOY 020/0000z - 020/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 17310 | Michael Koss, Eureka Scientific Inc. | A Blue Gap Survey of Nearby Active Galaxies |
| 17491 | Grace Telford, Princeton University | A Legacy Far-Ultraviolet Spectral Atlas of Extremely Metal-Poor O Stars |
| 17509 | Christina Lindberg, The Johns Hopkins University | Winging the SMC: 3D Structure of the Interstellar Medium in the Tidally Distrupted Wing of the SMC |
| 17696 | Kevin France, University of Colorado at Boulder | Can NUV Flares Kickstart Prebiotic Chemical Chains on M Dwarf Planets? |
| 17697 | Matti Dorsch, Universitat Potsdam | A far-UV treasury survey for hot subdwarf stars |
| 17698 | Boris Gaensicke, University of Warwick | A legacy survey for evolved planetary systems within 100pc |
| 17718 | Filippo D'Ammando, INAF Istituto di Radioastronomia | Uncovering the host galaxy and BH mass of a large sample of radio-loud narrow-line Seyfert 1 galaxies |
| 17735 | Adam Bolton, SLAC National Accelerator Laboratory | Confirming Spectroscopic Strong Lens Candidates from the DESI One-Percent Survey |
| 17794 | Sudeshna Boro Saikia, University of Vienna | FUV flux of nearby exoplanet host stars in the Ariel target list |
| Calibration Observations Scheduled | ||
| 17624 | Jacqueline Hernandez, Space Telescope Science Institute | Cycle 32 COS FUV Spectroscopic Sensitivity Monitor |
| 17629 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Dark Monitor Part 1 |
| 17632 | Joshua Lothringer, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
| 17653 | Alyssa Guzman, Space Telescope Science Institute | CCD Daily Monitor (Part 1) |
| 17667 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 1 |
| 17689 | Frederick Dauphin, Space Telescope Science Institute | WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |