| Earlier reports | Convert Day of Year |
Daily Report #8875
Period Covered:
08:00 PM October 30, 2020 - 07:59 PM October 31, 2020
(DOY 305/0000z - 305/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 15446 | Julianne Dalcanton, University of Washington | Establishing HST's Low Redshift Archive of Interacting Systems |
| 15828 | Aida Wofford, Universidad Nacional Autonoma de Mexico, Obs. Astron. Nac. | Essential observations of the stellar and nebular He II emission in two extreme metal-poor starbursts. |
| 15932 | Martha Boyer, Space Telescope Science Institute | Uncovering the Cause of the Shift in Carbon Star Behaviour at High Metallicity |
| 16162 | Martha Boyer, Space Telescope Science Institute | Solving the metallicity dependence of evolved star evolution and completing HST's near-IR legacy in the Local Volume |
| 16183 | Simon Porter, Southwest Research Institute | Followup High-Precision Astrometry and Binary Searches of Potential New Horizons KBO Targets |
| 16241 | Michael Koss, Eureka Scientific Inc. | A NUV Snapshot Survey of the Nearest Luminous AGN |
| 16261 | Sally Oey, University of Michigan | Mrk 71: Prototype for Catastrophic Cooling in a Green Pea Analog |
| 16269 | David Jones, University of California - Santa Cruz | Tension at the Breaking Point: Uncovering New Physics Through a Two-Rung Distance Ladder Measurement of the Hubble Constant |
| 16423 | Vivienne Baldassare, Washington State University | A CHANDRA LOOK AT VARIABILITY-SELECTED LOW-MASS AGN CANDIDATES |
| Calibration Observations Scheduled | ||
| 15713 | Heather Kurtz, Space Telescope Science Institute | UVIS Bowtie Monitor |
| 15716 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor Part 3 |
| 15737 | Matthew Maclay, Space Telescope Science Institute | STIS CCD Dark Monitor Part 3 |
| 15739 | Matthew Maclay, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
| 16412 | Jennifer Medina, Space Telescope Science Institute | WFC3 CSM Monitor with Earth Flats |