Earlier reports | Convert Day of Year |
Daily Report #6850
Period Covered:
08:00 pm April 15, 2015 - 07:59 pm April 16, 2015
(DOY 106/0000z - 106/2359z)
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 |
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