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Daily Report #7121
Period Covered:
07:00 pm January 11, 2016 - 06:59 pm January 12, 2016
(DOY 012/0000z - 012/2359z)
This report was generated by the HST Automated Report System @2016-01-13 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 |
13765 | Bradley Peterson, The Ohio State University | A Cepheid-Based Distance to the Benchmark AGN NGC 4151 |
13851 | Howard Bond, The Pennsylvania State University | The Origin of Intermediate-Luminosity Red Transients |
14076 | Boris Gaensicke, The University of Warwick | An HST legacy ultraviolet spectroscopic survey of the 13pc white dwarf sample |
14095 | Gabriel Brammer, Space Telescope Science Institute - ESA | Calibrating the Dusty Cosmos: Extinction Maps of Nearby Galaxies |
14216 | Robert Kirshner, Harvard University | RAISIN2: Tracers of cosmic expansion with SN IA in the IR |
14243 | Deirdre Coffey, University College Dublin | True Jet Rotation Probed in NUV Jet Core |
14262 | Knud Jahnke, Max-Planck-Institut fur Astronomie, Heidelberg | Are the fastest growing black holes at z=2 caused by major galaxy mergers? |
Calibration Observations Scheduled | ||
14368 | Matthew Bourque, Space Telescope Science Institute | WFC3 UVIS Daily Monitor A |
14381 | Knox Long, Eureka Scientific Inc. | WFC3 IR Persistence: Position Dependent Model |
14382 | Sylvia Baggett, Space Telescope Science Institute | WFC3/UVIS contamination and stability monitor |
14392 | Peter McCullough, Space Telescope Science Institute | WFC3 CSM monitor Earth Flats |
14400 | David Golimowski, Space Telescope Science Institute | CCD Hot Pixel Annealing |
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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