The Hubble Space Telescope
Unlocking the Secrets of the Universe
Daily Report #6598
Period Covered:
08:00 pm August 6, 2014 - 07:59 pm August 7, 2014
(DOY 219/0000z - 219/2359z)
Flight Operations Summary
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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