Earlier reports | Convert Day of Year |
Daily Report #10468
Period Covered:
08:00 PM March 11, 2025 - 07:59 PM March 12, 2025
(DOY 071/0000z - 071/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
17461 | Vihang Mehta, California Institute of Technology | Unlocking the rich potential of JWST slitless spectroscopy with the help of HST: an optical follow-up campaign |
17493 | Miriam Keppler, University of Arizona | Mapping the inner disk wind of RU Lup with molecular hydrogen |
17697 | Matti Dorsch, Universitat Potsdam | A far-UV treasury survey for hot subdwarf stars |
17754 | Helge Todt, Universitat Potsdam | Hydrogen-deficient central stars of planetary nebulae: testing the post-AGB evolution and s-process production |
17770 | Daichi Hiramatsu, Harvard University | Unveiling the Progenitors of Interacting Supernovae with Resolved Host Galaxy Imaging in the Rest-Frame UV |
17837 | Michael Tucker, The Ohio State University | Elevating the Scientific Output of JWST by using HST to Examine the Heart of Type Ia Supernova 2021aefx |
17883 | Christopher Britt, Space Telescope Science Institute | Broadband imaging of NGC 5335 |
17890 | Nissim Kanekar, National Centre for Radio Astrophysics, TIFR | The HI properties of low-z Green Pea galaxies |
17924 | Brent Smith, Arizona State University | TREASURETROVE: Tracing the Growth of SMBHs and Spheroids through Variability and Transients in the JWST NEP Time Domain Field |
Calibration Observations Scheduled | ||
17630 | Matthew Dallas, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
17632 | Joshua Lothringer, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
17654 | Alyssa Guzman, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
17657 | Alyssa Guzman, Space Telescope Science Institute | CCD Hot Pixel Annealing |
17667 | Aidan Pidgeon, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 1 |
17677 | Frederick Dauphin, Space Telescope Science Institute | WFC3 IR Dark Monitor |