Earlier reports | Convert Day of Year |
Daily Report #9768
Period Covered:
08:00 PM April 11, 2023 - 07:59 PM April 12, 2023
(DOY 102/0000z - 102/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
16689 | Kevin Burdge, Massachusetts Institute of Technology | Using STIS ultraviolet spectroscopy to understand the physical properties, evolution, and structure of white dwarfs in sixteen newly discovered ultracompact binaries. |
17108 | Justin Spilker, Texas A & M University | Dissecting Early Universe Dust with Matched-Resolution Observations from HST, JWST, and ALMA |
17153 | Floriane Leclercq, University of Texas at Austin | Resolving Lyman Alpha emission in a complete sample of Lyman Continuum leakers and non-leakers |
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 |
17216 | Alessandro Savino, University of California - Berkeley | Establishing a 1% anchor for the Population II Distance Ladder with HST and Gaia |
17269 | Xin Liu, University of Illinois at Urbana - Champaign | A Complete Census of Luminous Sub-arcsec Dual/Lensed Quasars at z > 1.5 |
17278 | Ryan Chornock, University of California - Berkeley | Testing the Limit: Late-time HST Observations of the Most Energetic GRB Ever |
Calibration Observations Scheduled | ||
16947 | Sophia Medallon, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
16949 | Sean Lockwood, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
16971 | Meaghan McDonald, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
17002 | Harish Khandrika, Space Telescope Science Institute | WFC3 UVIS Bowtie Monitor |
17004 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 2 |
17022 | Frederick Dauphin, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
17249 | Kate Rowlands, Space Telescope Science Institute | Cycle 30 COS FUV Spectroscopic Sensitivity Monitor |