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Daily Report #7311
Period Covered:
08:00 pm July 19, 2016 - 07:59 pm July 20, 2016
(DOY 202/0000z - 202/2359z)
This report was generated by the HST Automated Report System @2016-07-21 17:02:00 GMT
Significant Spacecraft Anomalies: (The following are preliminary reports of potential non-nominal performance that will be investigated.)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 14074 | Roger Cohen, Universidad de Concepcion | Opening the Window on Galaxy Assembly: Ages and Structural Parameters of Globular Clusters Towards the Galactic Bulge |
| 14121 | Edward Cackett, Wayne State University | Probing the accretion disk in the Seyfert 1 NGC 4593 |
| 14212 | Karl Stapelfeldt, Jet Propulsion Laboratory | A Snapshot Imaging Survey of Spitzer-selected Young Stellar Objects in Nearby Star Formation Regions*.t23 |
| 14219 | John Blakeslee, Dominion Astrophysical Observatory | Homogeneous Distances and Central Profiles for MASSIVE Survey Galaxies with Supermassive Black Holes |
| 14236 | Sangmo Sohn, Space Telescope Science Institute | The First Proper Motions of Ultra-faint Dwarf Galaxies: Probing Reionization and Planar Associations of Satellites |
| 14268 | Nicolas Lehner, University of Notre Dame | Project AMIGA: Mapping the Circumgalactic Medium of Andromeda |
| 14528 | Patrick Kelly, University of California - Berkeley | Caustic Crossing of a Strongly Lensed Massive Star |
| Calibration Observations Scheduled | ||
| 14370 | Matthew Bourque, Space Telescope Science Institute | WFC3 UVIS Daily Monitor C |
| 14397 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor (Part 3) |
| 14413 | Joanna Taylor, Space Telescope Science Institute | STIS CCD Dark Monitor Part 2 |
| 14415 | Joanna Taylor, Space Telescope Science Institute | CCD Bias and Read Noise Monitor Part 2 |
| 14441 | Joanna Taylor, Space Telescope Science Institute | NUV Spectroscopic Sensitivity Monitoring |
| 14504 | Julia Roman-Duval, Space Telescope Science Institute - ESA | Constraining the zero-points of the COS/NUV wavelength solution - G225M and G285M |
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