Earlier reports | Convert Day of Year |
Daily Report #10347
Period Covered:
07:00 PM November 10, 2024 - 06:59 PM November 11, 2024
(DOY 316/0000z - 316/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
17069 | Matthew Hayes, Stockholm University | The Lyman-alpha and Continuum Origins Survey (LaCOS) |
17309 | Vihang Mehta, California Institute of Technology | Resolved imaging survey of the analogs of high-z massive, star-forming clumps |
17436 | Joseph Jensen, Utah Valley University | An Independent High-Precision Distance Ladder for Cosmology |
17452 | Yuri Izotov, Ukrainian National Academy of Sciences, BITP | Lyman-alpha emission in low-mass compact galaxies with most extreme [OIII]5007/[OII]3727 ratios of above 30 |
17491 | Grace Telford, Princeton University | A Legacy Far-Ultraviolet Spectral Atlas of Extremely Metal-Poor O Stars |
17811 | Sebastian Gomez, Space Telescope Science Institute | Host Galaxy Imaging of Luminous Supernovae: The Missing Link of Stripped Envelope Core-Collapse Supernovae |
17881 | Meridith Joyce, University of Wyoming | Far-UV detection of the low-mass companion responsible for Betelgeuse's long secondary period |
Calibration Observations Scheduled | ||
17349 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
17351 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS Post-flash Monitor |
17629 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Dark Monitor Part 1 |
17632 | Joshua Lothringer, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
17653 | Alyssa Guzman, Space Telescope Science Institute | CCD Daily Monitor (Part 1) |
17666 | Harish Khandrika, Space Telescope Science Institute | WFC3 UVIS Bowtie Monitor |
17670 | Isabel Rivera, Space Telescope Science Institute | WFC3 UVIS CCD Unflashed (CTE) Monitor |
17671 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS Post-flash Monitor |
17689 | Frederick Dauphin, Space Telescope Science Institute | WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |