Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #6502

Period Covered:
08:00 pm May 2, 2014 - 07:59 pm May 3, 2014
(DOY 123/0000z - 123/2359z)

Flight Operations Summary

This report was generated by the HST Automated Report System @2014-05-04 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		5		5
FGS REAcq		5		5
OBAD with Maneuver	6		6

SIGNIFICANT EVENTS:
none


Program Principal Investigator Program Title
Science Observations Scheduled
12969 Peter Garnavich, University of Notre Dame Global Properties Are Not Enough: Probing the Local Environments of Type Ia Supernovae
13297 Giampaolo Piotto, Universita degli Studi di Padova The HST Legacy Survey of Galactic Globular Clusters: Shedding UV Light on Their Populations and Formation
13325 Claus Leitherer, Space Telescope Science Institute Pushing COS to the {Lyman-}Limit
13330 Bradley Peterson, The Ohio State University Mapping the AGN Broad Line Region by Reverberation
13352 Matthew Malkan, University of California - Los Angeles WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time
13491 Todd Tripp, University of Massachusetts - Amherst Directly Probing >10^6 K Gas in Lyman Limit Absorbers at z > 2
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
13557 Matthew Bourque, Space Telescope Science Institute UVIS CCD Daily Monitor B
13562 Michael Dulude, Space Telescope Science Institute IR Dark Monitor
13625 Knox Long, Space Telescope Science Institute Characterizing persistence following scanned grism observations with WFC3/IR