| Earlier reports | Convert Day of Year |
Daily Report #6598
Period Covered:
08:00 pm August 6, 2014 - 07:59 pm August 7, 2014
(DOY 219/0000z - 219/2359z)
This report was generated by the HST Automated Report System @2014-08-08 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 12 12 FGS REAcq 4 4 OBAD with Maneuver 8 8 SIGNIFICANT EVENTS: none
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 12903 | Luis Ho, Carnegie Institution of Washington | The Evolutionary Link Between Type 2 and Type 1 Quasars |
| 13331 | Laurent Pueyo, Space Telescope Science Institute | Confirmation and characterization of young planetary companions hidden in the HST NICMOS archive |
| 13433 | Justyn Maund, The Queen's University of Belfast | Stellar Forensics V: A post-explosion view of the progenitor of SN 2011dh |
| 13455 | John Krist, Jet Propulsion Laboratory | The Eccentric Debris Ring Around HD 202628: Signs of Planetary Perturbations |
| 13463 | Kailash Sahu, Space Telescope Science Institute | Detecting and Measuring the Masses of Isolated Black Holes and Neutron Stars through Astrometric Microlensing |
| 13496 | Jennifer Lotz, Space Telescope Science Institute | HST Frontier Fields - Observations of MACSJ0416.1-2403 |
| 13678 | Adam Riess, The Johns Hopkins University | The Fifth and Final Epoch |
| 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 |
| 13558 | Matthew Bourque, Space Telescope Science Institute | UVIS CCD Daily Monitor C |
| 13624 | Elena Sabbi, Space Telescope Science Institute | Monitoring Persistence in WFC3/IR after scanned grism observations |
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