Earlier reports | Convert Day of Year |
Daily Report #7243
Period Covered:
08:00 pm May 12, 2016 - 07:59 pm May 13, 2016
(DOY 134/0000z - 134/2359z)
This report was generated by the HST Automated Report System @2016-05-14 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 | ||
14076 | Boris Gaensicke, The University of Warwick | An HST legacy ultraviolet spectroscopic survey of the 13pc white dwarf sample |
14090 | Gilda Ballester, University of Arizona | New FUV diagnostics of the atmosphere of the hot-Jupiter HD 209458b with HST/COS |
14133 | David Polishook, Weizmann Institute of Science | Establishing an evolutionary sequence for disintegrated minor planets |
14151 | Anna Frebel, Massachusetts Institute of Technology | Constraining Pop III supernova energies and the formation of the first low-mass stars with the iron-poor star HE1327-2326 (with [Fe/H] = -5.4) |
14178 | Matthew Malkan, University of California - Los Angeles | WFC3 Infrared Spectroscopic Parallel Survey: The WISP Deep Fields |
14199 | Patrick Kelly, University of California - Berkeley | Refsdal Redux: Precise Measurements of the Reappearance of the First Supernova with Multiple Resolved Images |
14235 | Sangmo Sohn, The Johns Hopkins University | Globular Cluster Orbits from HST Proper Motions: Constraining the Formation and Mass of the Milky Way Halo |
Calibration Observations Scheduled | ||
14367 | Meredith Durbin, Space Telescope Science Institute | UVIS Bowtie Monitor |
14369 | Matthew Bourque, Space Telescope Science Institute | WFC3 UVIS Daily Monitor B |
14380 | Knox Long, Eureka Scientific Inc. | WFC3 IR Persistence: Amplitude Variations |
14396 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
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 |
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