Earlier reports | Convert Day of Year |
Daily Report #6169
Period Covered:
08:00 pm June 3, 2013 - 07:59 pm June 4, 2013
(DOY 155/0000z - 155/2359z)
This report was generated by the HST Automated Report System @2013-06-05 17:02:02 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 10 10 FGS REAcq 5 5 OBAD with Maneuver 8 8 SIGNIFICANT EVENTS: none
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
12938 | Sergio Dieterich, Georgia State University Research Foundation | Probing Fundamental Stellar Parameters with HST/STIS Spectroscopy of M Dwarf Binaries |
12939 | Elena Sabbi, Space Telescope Science Institute - ESA | Hubble Tarantula Treasury Project {HTTP: unraveling Tarantula's web} |
12942 | Eilat Glikman, Yale University | Testing the Merger Hypothesis for Black Hole/Galaxy Co-Evolution at z~2 |
12972 | Christopher Gelino, Jet Propulsion Laboratory | In Search of the Coldest Atmospheres: Identifying Companions to the Latest WISE Brown Dwarfs |
12990 | Adam Muzzin, Sterrewacht Leiden | Size Growth at the Top: WFC3 Imaging of Ultra-Massive Galaxies at 1.5 < z < 3 |
13015 | Karen Leighly, University of Oklahoma Norman Campus | WPVS 007: Acceleration or Evolution in a Broad Absorption Line Outflow |
13063 | Adam Riess, The Johns Hopkins University | Supernova Follow-up for MCT |
Calibration Observations Scheduled | ||
13072 | Matthew Bourque, Space Telescope Science Institute | UVIS Bowtie Monitor |
13075 | John Biretta, Space Telescope Science Institute | UVIS CCD Daily Monitor C |
13084 | Elena Sabbi, Space Telescope Science Institute - ESA | Characterization of UVIS Traps with CI |
13132 | Svea Hernandez, Space Telescope Science Institute | CCD Dark Monitor Part 2 |
13151 | Svea Hernandez, Space Telescope Science Institute | CCD Bias and Read Noise Monitor-Part 2 |
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