| Earlier reports | Convert Day of Year |
Daily Report #9955
Period Covered:
08:00 PM October 15, 2023 - 07:59 PM October 16, 2023
(DOY 289/0000z - 289/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 16489 | Noel Castro Segura, University of Southampton | Outflow Legacy Accretion Survey: unveiling the wind driving mechanism in BHXRBs |
| 16701 | Allison Youngblood, NASA Goddard Space Flight Center | Essential Ultraviolet Stellar Characterization for Cycle 1 JWST Transiting Planet Targets |
| 16773 | Karl Glazebrook, Swinburne University of Technology | A SNAPshot Legacy Survey of Bright Gravitational Lenses |
| 17110 | David Setton, University of Pittsburgh | Post-starbursts from DESI: Timing quenching and morphological transformation at 1 < z < 1.3 |
| 17115 | David Bowen, Princeton University | The Circumgalactic Medium of Dwarf Galaxy Pairs |
| 17147 | Claudia Scarlata, University of Minnesota - Twin Cities | The Parallel Ionizing Emissivity Survey |
| 17217 | Gabor Worseck, Private Company | The First Dedicated Spectroscopic Extreme UV Survey of Low-Luminosity Broad-Line Active Galactic Nuclei |
| 17227 | Todd Tripp, University of Massachusetts - Amherst | Unique Constraints on the Physics of Circumgalactic Gas from Ultrahigh Resolution Observations of Galactic High-Velocity Clouds |
| 17276 | Ingrid Pelisoli, The University of Warwick | A new radio pulsing white dwarf? |
| Calibration Observations Scheduled | ||
| 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 |
| 16972 | Meaghan McDonald, Space Telescope Science Institute | CCD Daily Monitor (Part 3) |
| 17005 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
| 17006 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Unflashed (CTE) Monitor |
| 17019 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |