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Daily Report #5304
Period Covered:
07:00 pm January 20, 2011 - 06:59 pm January 21, 2011
(DOY 21/0000z - 21/2359z)
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 8 8 SIGNIFICANT EVENTS: none
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
11597 | S. Stanford, University of California - Davis | Spectroscopy of IR-Selected Galaxy Clusters at 1 < z < 1.5 |
11696 | Matthew Malkan, University of California - Los Angeles | Infrared Survey of Star Formation Across Cosmic Time |
11705 | Frederick Hamann, University of Florida | Physical Properties of Quasar Outflows: From BALs to mini-BALs |
12166 | Harald Ebeling, University of Hawaii | A Snapshot Survey of The Most Massive Clusters of Galaxies |
12184 | Xiaohui Fan, University of Arizona | A SNAP Survey for Gravitational Lenses Among z~6 Quasars |
12197 | Johan Richard, University of Durham | Evolution in the Size-Luminosity Relation of HII regions in Gravitationally-lensed galaxies |
12203 | S. Stanford, University of California - Davis | Rest Frame Optical Spectroscopy of Galaxy Clusters at 1.6 < z < 1.9 |
12319 | Slawomir Piatek, New Jersey Institute of Technology | Proper Motion Survey of Classical and SDSS Local Group Dwarf Galaxies |
Calibration Observations Scheduled | ||
12342 | Tiffany Borders, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor |
12355 | Norbert Pirzkal, Space Telescope Science Institute | IR Grism Wavelength and LSF Calibration |
12358 | Howard Bushouse, Space Telescope Science Institute | IR Grism L-Flat Correction and Independent 2-D Wavelength Solution |
12384 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor {Part 1} |
12400 | Michael Wolfe, Space Telescope Science Institute | Dark Monitor Part 1 |
12402 | Michael Wolfe, Space Telescope Science Institute | CCD Bias and Read Noise Monitor-Part 1 |