Earlier reports | Convert Day of Year |
Daily Report #10109
Period Covered:
08:00 PM March 17, 2024 - 07:59 PM March 18, 2024
(DOY 078/0000z - 078/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
16658 | Jessica Lu, University of California - Berkeley | Hunting for Black Holes with Astrometric Microlensing |
17145 | William Harris, McMaster University | Clearing a Window Into Galaxy Formation: The Impact of Globular Cluster Metallicity Distributions |
17436 | Joseph Jensen, Utah Valley University | An Independent High-Precision Distance Ladder for Cosmology |
17440 | Elisa Garro, European Southern Observatory - Chile | Assembling the Milky Way: Adding Globular Clusters from the Sagittarius Dwarf Galaxy |
17446 | Peter Milne, University of Arizona | Extending Precision Cosmology to Early Hosts of Type Ia Supernovae via Surface Brightness Fluctuation (SBF) Distances |
17449 | Giorgos Leloudas, Technical University of Denmark-DTU Space | Early spectroscopy of tidal disruption events: outflow signatures or chemical composition ? |
17504 | Patrick Kelly, University of Minnesota - Twin Cities | SNAP Survey for Strongly Lensed Supernovae and Magnified Stars |
17603 | Justyn Maund, Royal Holloway, University of London | Did the progenitor of the Type IIb SN2011dh actually have a binary companion? |
Calibration Observations Scheduled | ||
17334 | Meaghan McDonald, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
17338 | Roberto Avila, Space Telescope Science Institute | ACS SBC Photometric Monitor |
17347 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 1 |
17371 | Frederick Dauphin, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |
17375 | Sophia Medallon, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
17377 | Daniel Stapleton, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
17379 | Sophia Medallon, Space Telescope Science Institute | STIS CCD Hot Pixel Annealing |