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Daily Report #6536
Period Covered:
08:00 pm June 5, 2014 - 07:59 pm June 6, 2014
(DOY 157/0000z - 157/2359z)
This report was generated by the HST Automated Report System @2014-06-07 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 6 6 FGS REAcq 9 9 OBAD with Maneuver 6 6 SIGNIFICANT EVENTS: none
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
13280 | Esther Buenzli, Max-Planck-Institut fur Astronomie, Heidelberg | Evolution of heterogeneous cloud structure through the T dwarf sequence |
13305 | Carolin Villforth, University of St. Andrews | Do mergers matter? Testing AGN triggering mechanisms from Seyferts to Quasars |
13330 | Bradley Peterson, The Ohio State University | Mapping the AGN Broad Line Region by Reverberation |
13347 | Joel Bregman, University of Michigan | The Missing Baryons Around Nearby Dwarf Galaxies |
13382 | Mary Putman, Columbia University in the City of New York | Warm Gas Flows in the Coma Cluster |
13393 | Dennis Zaritsky, University of Arizona | Galaxy Transformation in the Infall Regions of Clusters |
13517 | Matthew Malkan, University of California - Los Angeles | WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time |
Calibration Observations Scheduled | ||
13519 | Svea Hernandez, Space Telescope Science Institute | CCD Dark Monitor Part 2 |
13521 | Justin Ely, Space Telescope Science Institute | FUV Detector Dark Monitor |
13536 | Svea Hernandez, Space Telescope Science Institute | CCD Bias and Read Noise Monitor-Part 2 |
13557 | Matthew Bourque, Space Telescope Science Institute | UVIS CCD Daily Monitor B |
13590 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor {Part 2} |
13594 | David Golimowski, Space Telescope Science Institute | CCD Hot Pixel Annealing |
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