Earlier reports | Convert Day of Year |
Daily Report #9833
Period Covered:
08:00 PM June 15, 2023 - 07:59 PM June 16, 2023
(DOY 167/0000z - 167/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
17067 | Gaspard Duchene, University of California - Berkeley | The diversity of protoplanetary disks: Imaging a complete sample of edge-on disks in four nearby star-forming regions |
17128 | Ryan Foley, University of California - Santa Cruz | Reducing Type Ia Supernova Distance Biases by Separating Reddening and Intrinsic Color |
17130 | Tommaso Treu, University of California - Los Angeles | A 4% determination of the Hubble constant from gravitational time delays with maximally flexible lens mass profile |
17153 | Floriane Leclercq, University of Texas at Austin | Resolving Lyman Alpha emission in a complete sample of Lyman Continuum leakers and non-leakers |
17162 | David Sing, The Johns Hopkins University | The HST/JWST synergy: A deep dive into the NUV with WASP-39b to answer key formation questions |
17177 | Igor Chilingarian, Smithsonian Institution Astrophysical Observatory | Snapshot survey of host galaxies of active 'light-weight' supermassive black holes |
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 |
17180 | Svea Hernandez, Space Telescope Science Institute - ESA - JWST | What's hidding in the neutral gas? Dissecting the different metallicity components in NGC 1313 |
Calibration Observations Scheduled | ||
16947 | Sophia Medallon, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
16950 | Sean Lockwood, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
16971 | Meaghan McDonald, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
17004 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 2 |
17006 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Unflashed (CTE) Monitor |