Earlier reports | Convert Day of Year |
Daily Report #7072
Period Covered:
07:00 pm November 23, 2015 - 06:59 pm November 24, 2015
(DOY 328/0000z - 328/2359z)
This report was generated by the HST Automated Report System @2015-11-25 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 | ||
13711 | Abhijit Saha, National Optical Astronomy Observatory, AURA | Establishing a Network of Next Generation SED standards with DA White Dwarfs |
13801 | Varsha Kulkarni, University of South Carolina Research Foundation | Probing Structure in Cold Gas at z <~ 1 with Gravitationally Lensed Quasar Sightlines |
14054 | Ehud Behar, Technion-Israel Institute of Technology | Tracking Down the Ionized Outflow of NGC 7469 |
14119 | Luciana Bianchi, The Johns Hopkins University | Understanding Stellar Evolution of Intermediate-Mass Stars from a New Sample of SiriusB-Like Binaries |
14141 | Guy Worthey, Washington State University | NGSL Extension 1. Hot Stars and Evolved Stars |
14241 | Daniel Apai, University of Arizona | Cloud Atlas: Vertical Cloud Structure and Gravity in Exoplanet and Brown Dwarf Atmospheres |
14262 | Knud Jahnke, Max-Planck-Institut fur Astronomie, Heidelberg | Are the fastest growing black holes at z=2 caused by major galaxy mergers? |
14268 | Nicolas Lehner, University of Notre Dame | Project AMIGA: Mapping the Circumgalactic Medium of Andromeda |
Calibration Observations Scheduled | ||
14367 | Meredith Durbin, Space Telescope Science Institute | UVIS Bowtie Monitor |
14368 | Matthew Bourque, Space Telescope Science Institute | WFC3 UVIS Daily Monitor A |
14392 | Peter McCullough, Space Telescope Science Institute | WFC3 CSM monitor Earth Flats |
14412 | Joanna Taylor, Space Telescope Science Institute | CCD Dark Monitor Part 1 |
14414 | Joanna Taylor, Space Telescope Science Institute | CCD Bias and Read Noise Monitor Part 2 |
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