Earlier reports Convert Day of Year

The Hubble Space Telescope

Unlocking the Secrets of the Universe

Daily Report #6850

Period Covered:
08:00 pm April 15, 2015 - 07:59 pm April 16, 2015
(DOY 106/0000z - 106/2359z)

Flight Operations Summary

This report was generated by the HST Automated Report System @2015-04-17 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		9		9
FGS REAcq		8		8
OBAD with Maneuver	8		8

SIGNIFICANT EVENTS:
none


Program Principal Investigator Program Title
Science Observations Scheduled
13772 Martin Weisskopf, NASA Marshall Space Flight Center Joint Chandra and HST Monitoring and Studies of the Crab Nebula
13776 Michael Gregg, University of California - Davis Completing The Next Generation Spectral Library
13847 Kailash Sahu, Space Telescope Science Institute Determining the Mass of Proxima Centauri through Astrometric Microlensing
14056 Zolt Levay, Space Telescope Science Institute Veil Nebula mosaic
Calibration Observations Scheduled
13967 Hugues Sana, Space Telescope Science Institute - ESA COS FUV Spectroscopic Sensitivity Monitoring
13971 David Sahnow, Space Telescope Science Institute COS FUV Channel Sensitivity vs. High Voltage
13973 Joanna Taylor, Space Telescope Science Institute NUV Spectroscopic Sensitivity Monitoring
13980 Joanna Taylor, Space Telescope Science Institute CCD Dark Monitor Part 1
13982 Joanna Taylor, Space Telescope Science Institute CCD Bias and Read Noise Monitor Part 1
13984 Joanna Taylor, Space Telescope Science Institute STIS CCD Hot Pixel Annealing
14001 Meredith Durbin, Space Telescope Science Institute UVIS Bowtie Monitor
14003 Matthew Bourque, Space Telescope Science Institute WFC3 UVIS Daily Monitor B
14014 Elena Sabbi, Space Telescope Science Institute WFC3 UVIS Traps with CI
14015 Knox Long, Eureka Scientific Inc. Refining the WFC3/IR Persistence model