| Earlier reports | Convert Day of Year |
Daily Report #7990
Period Covered:
08:00 PM May 29, 2018 - 07:59 PM May 30, 2018
(DOY 150/0000z - 150/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 15085 | Robert Simcoe, Massachusetts Institute of Technology | Galaxies in the Diffuse Baryon Field Approaching Reionization: A Joint Study with JWST, HST, and Large Telescopes |
| 15111 | Pippa Molyneux, Southwest Research Institute | The UV reflectance of Patroclus: Exploring the surface composition and origins of Jupiter Trojans |
| 15163 | Hsiao-Wen Chen, University of Chicago | COS Ultraviolet Baryon Survey (CUBS) |
| 15166 | Alex Filippenko, University of California - Berkeley | Continuing a Snapshot Survey of the Sites of Recent, Nearby Supernovae: Cycles 25 & 26 |
| 15201 | Clemence Fontanive, Royal Observatory Edinburgh | Looking for the Coldest Atmospheres: a Search for Planetary Mass Companions around T and Y Brown Dwarfs |
| 15261 | Anne Verbiscer, The University of Virginia | The Pluto System in the Post-New Horizons Era: Opposition Effects, Rotations, and Orbital Stability |
| 15323 | Jonelle Walsh, Texas A & M University | Addressing a Bias in the Galaxies with Black Hole Mass Measurements |
| Calibration Observations Scheduled | ||
| 14947 | Tyler Desjardins, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
| 14951 | Tyler Desjardins, Space Telescope Science Institute | CCD Hot Pixel Annealing |
| 14960 | Allyssa Riley, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
| 14963 | Allyssa Riley, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
| 14979 | Heather Kurtz, Space Telescope Science Institute | UVIS Bowtie Monitor |
| 14981 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS Daily Monitor B |
| 14996 | Myles Mckay, Space Telescope Science Institute | WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats Monitor |
| 14999 | Ben Sunnquist, Space Telescope Science Institute | WFC3 CSM monitor with earth flats |
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