| Earlier reports | Convert Day of Year |
Daily Report #6502
Period Covered:
08:00 pm May 2, 2014 - 07:59 pm May 3, 2014
(DOY 123/0000z - 123/2359z)
This report was generated by the HST Automated Report System @2014-05-04 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 5 5 FGS REAcq 5 5 OBAD with Maneuver 6 6 SIGNIFICANT EVENTS: none
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 12969 | Peter Garnavich, University of Notre Dame | Global Properties Are Not Enough: Probing the Local Environments of Type Ia Supernovae |
| 13297 | Giampaolo Piotto, Universita degli Studi di Padova | The HST Legacy Survey of Galactic Globular Clusters: Shedding UV Light on Their Populations and Formation |
| 13325 | Claus Leitherer, Space Telescope Science Institute | Pushing COS to the {Lyman-}Limit |
| 13330 | Bradley Peterson, The Ohio State University | Mapping the AGN Broad Line Region by Reverberation |
| 13352 | Matthew Malkan, University of California - Los Angeles | WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time |
| 13491 | Todd Tripp, University of Massachusetts - Amherst | Directly Probing >10^6 K Gas in Lyman Limit Absorbers at z > 2 |
| Calibration Observations Scheduled | ||
| 13519 | Svea Hernandez, Space Telescope Science Institute | CCD Dark Monitor Part 2 |
| 13536 | Svea Hernandez, Space Telescope Science Institute | CCD Bias and Read Noise Monitor-Part 2 |
| 13555 | Matthew Bourque, Space Telescope Science Institute | UVIS Bowtie Monitor |
| 13557 | Matthew Bourque, Space Telescope Science Institute | UVIS CCD Daily Monitor B |
| 13562 | Michael Dulude, Space Telescope Science Institute | IR Dark Monitor |
| 13625 | Knox Long, Space Telescope Science Institute | Characterizing persistence following scanned grism observations with WFC3/IR |