Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #6275

Period Covered:
08:00 pm September 17, 2013 - 07:59 pm September 18, 2013
(DOY 261/0000z - 261/2359z)

Flight Operations Summary

This report was generated by the HST Automated Report System @2013-09-19 17:02:02 GMT

Significant Spacecraft Anomalies: (The following are preliminary reports
of potential non-nominal performance that will be investigated.)

HSTARs:
13815 - SCI: GSAcq (1,2,2) resiulted in FLBU (1,0,1)@261/1954z

COMPLETED OPS REQUEST:
none

COMPLETED OPS NOTES:
none

FGS ACQ STATUS:
		    SCHEDULED       SUCCESSFUL
FGS GSAcq		7		7
FGS REAcq		8		7
OBAD with Maneuver	7		7

SIGNIFICANT EVENTS:
none


Program Principal Investigator Program Title
Science Observations Scheduled
12937 Dennis Zaritsky, University of Arizona Direct Confirmation of Intracluster Stars as SN Ia Progenitors
12974 Matthew Mechtley, Arizona State University WFC3IR Imaging of UV-Faint z=6 Quasars: Star-Forming Host Galaxies of AGN in the Early Universe
13047 John Clarke, Boston University The D/H Ratio and Escape of Water from Venus
13364 Daniela Calzetti, University of Massachusetts - Amherst LEGUS: Legacy ExtraGalactic UV Survey
13388 Gregory Schwarz, American Astronomical Society Fundamental properties of novae outburst: Coordinated HST and XMM ToO observations
13400 Arlin Crotts, Columbia University in the City of New York The Surprising Ejecta Geometry of Recurrent Nova T Pyx
Calibration Observations Scheduled
13076 John Biretta, Space Telescope Science Institute UVIS CCD Daily Monitor D
13119 Azalee Bostroem, Space Telescope Science Institute COS FUV Spectroscopic Sensitivity Monitoring
13132 Svea Hernandez, Space Telescope Science Institute CCD Dark Monitor Part 2
13151 Svea Hernandez, Space Telescope Science Institute CCD Bias and Read Noise Monitor-Part 2
13154 David Golimowski, Space Telescope Science Institute CCD Daily Monitor {Part 3}
13499 Peter McCullough, Space Telescope Science Institute WFC3 Blob Monitor Using Dark-Earth IR Flats