Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #6522

Period Covered:
08:00 pm May 22, 2014 - 07:59 pm May 23, 2014
(DOY 143/0000z - 143/2359z)

Flight Operations Summary

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