Earlier reports | Convert Day of Year |
Daily Report #10315
Period Covered:
08:00 PM October 09, 2024 - 07:59 PM October 10, 2024
(DOY 284/0000z - 284/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
17308 | Cameron Lemon, Oskar Klein Centre, Stockholm University | An HST Gap Program for lensed Quasars |
17420 | Boris Gaensicke, University of Warwick | A legacy survey for evolved planetary systems within 100pc |
17433 | Qiaoya Wu, University of Illinois at Urbana - Champaign | HST UV Spectroscopy of High-accretion-rate AGNs and the Origin of Offset in the Broad-Line Region Size-Luminosity Relation |
17474 | Justin Pierel, Space Telescope Science Institute | Pioneering Precision: Advancing Cosmology with the First Statistical Sample of Gravitationally Lensed Supernovae |
17483 | Rajeshwari Dutta, Inter-University Centre for Astronomy and Astrophysics | Characterizing Lyman-Alpha emitters with Snapshot Survey (CLASS) |
17518 | Alexander Beckett, Space Telescope Science Institute | PIE+: Identifying LyC leakers through improved photometry of the PIE survey fields |
17530 | Lee Patrick, Centro de Astrobiologia (CSIC/INTA) Inst. Nac. de Tec. Aero. | Hot and cool - hot companions as probes of red supergiants |
17846 | Or Graur, University of Portsmouth | Tripling the sample of late-time Type Ia supernovae |
Calibration Observations Scheduled | ||
17324 | Christian Johnson, Space Telescope Science Institute | Cycle 31 FUV Detector Dark Monitor |
17349 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
17354 | Benjamin Kuhn, Space Telescope Science Institute | WFC3 UVIS CTE Monitor (Star Cluster) |
17376 | Daniel Welty, Space Telescope Science Institute | STIS CCD Dark Monitor Part 3 |
17378 | Daniel Stapleton, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
Other Observations Scheduled | ||
15962 | Merle Reinhart, Space Telescope Science Institute | Routine EEPROM dumps for ACS, COS, STIS, and WFC3 |