Earlier reports | Convert Day of Year |
Daily Report #9825
Period Covered:
08:00 PM June 07, 2023 - 07:59 PM June 08, 2023
(DOY 159/0000z - 159/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
16245 | Goeran Oestlin, Stockholm University | Mapping Lyman alpha and ionization in the leakiest galaxies |
16705 | Doron Chelouche, University of Haifa | Shedding light on light echoes: mapping the accretion disk and broad line region in Mrk 279 |
17069 | Matthew Hayes, Stockholm University | The Lyman-alpha and Continuum Origins Survey (LaCOS) |
17108 | Justin Spilker, Texas A & M University | Dissecting Early Universe Dust with Matched-Resolution Observations from HST, JWST, and ALMA |
17116 | Joel Bregman, University of Michigan | The Hot Multi-Temperature Gaseous Halos of Galaxies and Groups |
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 |
17137 | Dominik Riechers, Universitat zu Koln | Rise of the Titans: Stellar Properties of a Binary Hyper-Luminous Starburst Within the First Billion Years |
17147 | Claudia Scarlata, University of Minnesota - Twin Cities | The Parallel Ionizing Emissivity Survey |
17159 | Xin Wang, Chinese Academy of Sciences | Escaping Lyman Continuum from the Overdensities of Extreme Emission Line Galaxies at z~2.2 |
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 |
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 |
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 |