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Daily Report #6765
Period Covered:
07:00 pm January 20, 2015 - 06:59 pm January 21, 2015
(DOY 021/0000z - 021/2359z)
This report was generated by the HST Automated Report System @2015-01-22 17:02:00 GMT
Significant Spacecraft Anomalies: (The following are preliminary reports of potential non-nominal performance that will be investigated.) HSTARs: none COMPLETED OPS REQUEST: none COMPLETED OPS NOTES: none FGS ACQ STATUS: SCHEDULED SUCCESSFUL FGS GSAcq 7 7 FGS REAcq 8 8 OBAD with Maneuver 7 7 SIGNIFICANT EVENTS: none
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
13718 | Julie Wardlow, University of Copenhagen, Niels Bohr Institute | The nature and environment of the earliest dusty starburst galaxies |
13739 | Evan Skillman, University of Minnesota - Twin Cities | Is the First Epoch of Star Formation in Satellite Galaxies Universal? - Part II |
13772 | Martin Weisskopf, NASA Marshall Space Flight Center | Joint Chandra and HST Monitoring and Studies of the Crab Nebula |
13811 | Elisa Costantini, Space Research Organization Netherlands | Feedback in action in the type 1 Seyfert IZw 1 |
13868 | Dale Kocevski, Colby College | Are Compton-Thick AGN the Missing Link Between Mergers and Black Hole Growth? |
13872 | Pascal Oesch, Yale University | The GOODS UV Legacy Fields: A Full Census of Faint Star-Forming Galaxies at z~0.5-2 |
14040 | David Jewitt, University of California - Los Angeles | Unique Hubble Investigation of a Newly Discovered Main Belt Comet |
Calibration Observations Scheduled | ||
13952 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor (Part 1) |
13980 | Joanna Taylor, Space Telescope Science Institute | CCD Dark Monitor Part 1 |
13982 | Joanna Taylor, Space Telescope Science Institute | CCD Bias and Read Noise Monitor Part 1 |
14002 | Matthew Bourque, Space Telescope Science Institute | WFC3 UVIS Daily Monitor A |
14008 | Meredith Durbin, Space Telescope Science Institute | IR Dark Monitor |
14029 | Russell Ryan, Space Telescope Science Institute | IR internal flats |
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