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Daily Report #6522
Period Covered:
08:00 pm May 22, 2014 - 07:59 pm May 23, 2014
(DOY 143/0000z - 143/2359z)
This report was generated by the HST Automated Report System @2014-05-24 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 11 11 FGS REAcq 5 5 OBAD with Maneuver 8 8 SIGNIFICANT EVENTS: none
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 13330 | Bradley Peterson, The Ohio State University | Mapping the AGN Broad Line Region by Reverberation |
| 13344 | Adam Riess, The Johns Hopkins University | A 1% Measurement of the Distance Scale with Perpendicular Spatial Scanning |
| 13410 | Cristina Pallanca, Universita di Bologna | COSMIC-LAB: a BSS orbiting a NS? The companion to the supermassive NS in NGC6440. |
| 13463 | Kailash Sahu, Space Telescope Science Institute | Detecting and Measuring the Masses of Isolated Black Holes and Neutron Stars through Astrometric Microlensing |
| 13495 | Jennifer Lotz, Space Telescope Science Institute | HST Frontier Fields - Observations of Abell 2744 |
| Calibration Observations Scheduled | ||
| 13519 | Svea Hernandez, Space Telescope Science Institute | CCD Dark Monitor Part 2 |
| 13521 | Justin Ely, Space Telescope Science Institute | FUV Detector Dark Monitor |
| 13536 | Svea Hernandez, Space Telescope Science Institute | CCD Bias and Read Noise Monitor-Part 2 |
| 13557 | Matthew Bourque, Space Telescope Science Institute | UVIS CCD Daily Monitor B |
| 13575 | Susana Deustua, Space Telescope Science Institute | WFC3 UVIS & IR photometry |
| 13590 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor {Part 2} |
| 13622 | Merle Reinhart, Space Telescope Science Institute | FGS1R 15 Points of Light |
| 13624 | Elena Sabbi, Space Telescope Science Institute | Monitoring Persistence in WFC3/IR after scanned grism observations |
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