| Earlier reports | Convert Day of Year |
Daily Report #5247
Period Covered:
07:00 pm November 24, 2010 - 06:59 pm November 25, 2010
(DOY 329/0000z - 329/2359z)
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 5 5 FGS REAcq 9 9 OBAD with Maneuver 5 5 SIGNIFICANT EVENTS: none
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 11585 | Neil Crighton, Max-Planck-Institut fur Astronomie, Heidelberg | Tracing the distribution of gas and galaxies using three closely-spaced background QSOs |
| 11700 | Michele Trenti, University of Colorado at Boulder | Bright Galaxies at z>7.5 with a WFC3 Pure Parallel Survey |
| 11702 | Hao-Jing Yan, The Ohio State University | Search for Very High-z Galaxies with WFC3 Pure Parallel |
| 11741 | Todd Tripp, University of Massachusetts | Probing Warm-Hot Intergalactic Gas at 0.5 < z < 1.3 with a Blind Survey for O VI, Ne VIII, Mg X, and Si XII Absorption Systems |
| 12019 | Christy Tremonti, University of Wisconsin - Madison | After the Fall: Fading AGN in Post-starburst Galaxies |
| 12181 | Drake Deming, NASA Goddard Space Flight Center | The Atmospheric Structure of Giant Hot Exoplanets |
| 12307 | Andrew Levan, The University of Warwick | A public SNAPSHOT survey of gamma-ray burst host galaxies |
| 12329 | Linhua Jiang, University of Arizona | Physical Properties of Spectroscopically Confirmed Galaxies at 5.7 |
| Calibration Observations Scheduled | ||
| 11929 | Bryan Hilbert, Space Telescope Science Institute | IR Dark Current Monitor |
| 12337 | Abhijith Rajan, Space Telescope Science Institute | UVIS Internal Flats |
| 12342 | Tiffany Borders, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor |
| 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 |