| Earlier reports | Convert Day of Year |
Daily Report #5339
Period Covered:
07:00 pm February 24, 2011 - 06:59 pm February 25, 2011
(DOY 56/0000z - 56/2359z)
Significant Spacecraft Anomalies: (The following are preliminary reports of potential non-nominal performance that will be investigated.) HSTARs: 12721 - SCI: GSAcq(1,3,1) scheduled at 056/08:34:47, REAcq(1,3,1) scheduled at 056/10:10:02, at 11:45:53, at 13:25:29 and at 15:05:15 all results in Fine Lock Backup (1,0,1)@056/0841z Observations Possible affected: ACS 73 -88, Proposal ID#12253. COMPLETED OPS REQUEST: none COMPLETED OPS NOTES: 2129-1 - SCI: Modify COS FUV MAX HV operating limits (proposal12432@56/1842z FGS ACQ STATUS: SCHEDULED SUCCESSFUL FGS GSAcq 7 7 FGS REAcq 9 9 OBAD with Maneuver 7 7 SIGNIFICANT EVENTS: none
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 12161 | David Ardila, Jet Propulsion Laboratory | Accretion in Close Pre-Main-Sequence Binaries |
| 12215 | Nancy Evans, Smithsonian Institution Astrophysical Observatory | Searching for the Missing Low-Mass Companions of Massive Stars |
| 12253 | Douglas Clowe, Ohio University | Gravity in the Crossfire: Revealing the Properties of Dark Matter in Bullet-like Clusters |
| 12261 | Herman Marshall, Massachusetts Institute of Technology | Resolving the Pictor A Jet |
| 12278 | Thomas Ayres, University of Colorado at Boulder | Advanced Spectral Library Project: Cool Stars |
| 12320 | Brian Chaboyer, Dartmouth College | The Ages of Globular Clusters and the Population II Distance Scale |
| Calibration Observations Scheduled | ||
| 12342 | Tiffany Borders, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor |
| 12384 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor {Part 1} |
| 12392 | Ralph Bohlin, Space Telescope Science Institute | Photometric Cross-Calibration using Stellar Flux Standards |
| 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 |