| Earlier reports | Convert Day of Year |
Daily Report #9680
Period Covered:
07:00 PM January 13, 2023 - 06:59 PM January 14, 2023
(DOY 014/0000z - 014/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 15444 | Aaron Barth, University of California - Irvine | An ACS Schedule Gap Imaging Survey of Nearby Active Galaxies |
| 16686 | Daniel Weisz, University of California - Berkeley | The Metallicity Distribution Functions of Faint M31 Satellites |
| 16778 | Benjamin Williams, University of Washington | The Panchromatic Hubble Andromeda Southern Treasury (PHAST) |
| 17069 | Matthew Hayes, Stockholm University | The Lyman-alpha and Continuum Origins Survey (LaCOS) |
| 17083 | Viraj Karambelkar, California Institute of Technology | In search of the remnant of SN 2021fcg : detonation, deflagration or merger? |
| 17093 | Sanchayeeta Borthakur, Arizona State University | A Systematic Search for Wind-CGM Interactions in Star-forming Galaxies |
| 17128 | Ryan Foley, University of California - Santa Cruz | Reducing Type Ia Supernova Distance Biases by Separating Reddening and Intrinsic Color |
| 17140 | Francesca Annibali, INAF - OAS Bologna | Toward an observational test of the Lambda CDM hierarchical paradigm at the smallest galaxy scales |
| 17183 | Hannah Wakeford, University of Bristol | Hubble Ultraviolet-optical Survey of Transiting Legacy Exoplanets (HUSTLE) treasury program |
| Calibration Observations Scheduled | ||
| 16946 | Sophia Medallon, Space Telescope Science Institute | STIS CCD Dark Monitor Part 1 |
| 16949 | Doug Branton, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
| 17003 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 1 |
| 17011 | Frederick Dauphin, Space Telescope Science Institute | WFC3 IR Dark Monitor |
| 17022 | Frederick Dauphin, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
| 17261 | Debopam Som, Space Telescope Science Institute | WFC3 IR Time-Dependent Sensitivity: Spatial Scans |