Earlier reports | Convert Day of Year |
Daily Report #9870
Period Covered:
08:00 PM July 22, 2023 - 07:59 PM July 23, 2023
(DOY 204/0000z - 204/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
15446 | Julianne Dalcanton, University of Washington | Establishing HST's Low Redshift Archive of Interacting Systems |
17100 | Yuri Izotov, Ukrainian National Academy of Sciences, BITP | UV spectra of the most metal-deficient galaxies |
17121 | Varsha Kulkarni, University of South Carolina | Probing the Gas in and around Local Galaxies Mapped with Integral Field Spectroscopy |
17147 | Claudia Scarlata, University of Minnesota - Twin Cities | The Parallel Ionizing Emissivity Survey |
17179 | Lluis Galbany, Institute of Space Sciences (CSIC-IEEC) | A public HST-UV snapshot survey of type Ia supernova host galaxies with pre-existing optical integral-field spectroscopy |
17181 | Joseph Lyman, The University of Warwick | A public survey of superluminous supernovae hosts to study their progenitors |
17185 | Laura Rogers, University of Cambridge | How diverse is the bulk composition of exoplanetary material? |
17241 | Eileen Meyer, University of Maryland Baltimore County | Examining the Variability of High-Redshift Jets |
Calibration Observations Scheduled | ||
16935 | Christian Johnson, Space Telescope Science Institute | Cycle 30 COS NUV Detector Dark Monitor |
16948 | Sophia Medallon, Space Telescope Science Institute | STIS CCD Dark Monitor Part 3 |
16950 | Sean Lockwood, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
17002 | Harish Khandrika, Space Telescope Science Institute | WFC3 UVIS Bowtie Monitor |
17005 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
17015 | Annalisa Calamida, Space Telescope Science Institute | WFC3 UVIS and IR Photometry |
17022 | Frederick Dauphin, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
17251 | Kate Rowlands, Space Telescope Science Institute - ESA - JWST | Cycle 30 COS FUV Change in Spectroscopic Sensitivity Trends |