Earlier reports Convert Day of Year

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