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Daily Report #6082
Period Covered:
07:00 pm March 8, 2013 - 06:59 pm March 9, 2013
(DOY 068/0000z - 068/2359z)
This report was generated by the HST Automated Report System @2013-03-10 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 8 8 FGS REAcq 7 7 OBAD with Maneuver 6 6 SIGNIFICANT EVENTS: none
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
12870 | Boris Gaensicke, The University of Warwick | The mass and temperature distribution of accreting white dwarfs |
12883 | Denis Grodent, Universite de Liege | Unraveling electron acceleration mechanisms in Ganymede's space environment through N-S conjugate imagery of Jupiter's aurora |
12903 | Luis Ho, Carnegie Institution of Washington | The Evolutionary Link Between Type 2 and Type 1 Quasars |
12949 | Daniel Perley, California Institute of Technology | Unveiling the Dusty Universe with the Host Galaxies of Obscured GRBs |
13039 | Chris Simpson, Liverpool John Moores University | The environment of the z=7.085 QSO ULAS J1120+0641 |
Calibration Observations Scheduled | ||
13072 | Matthew Bourque, Space Telescope Science Institute | UVIS Bowtie Monitor |
13074 | John Biretta, Space Telescope Science Institute | UVIS CCD Daily Monitor B |
13078 | John Biretta, Space Telescope Science Institute | UVIS Post-Flash Monitor |
13083 | Kai Noeske, Space Telescope Science Institute | UVIS CTE Monitor {star clusters} |
13084 | Elena Sabbi, Space Telescope Science Institute - ESA | Characterization of UVIS Traps with CI |
13086 | Knox Long, Space Telescope Science Institute | WFC3 IR Persistance as a Function of Saturation Time |
13131 | Svea Hernandez, Space Telescope Science Institute | CCD Dark Monitor Part 1 |
13133 | Svea Hernandez, Space Telescope Science Institute | CCD Bias and Read Noise Monitor Part 1 |
13182 | David Hickey, Space Telescope Science Institute | WFC3 CSM Resolver using IR Earth Flats |