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Daily Report #5804
Period Covered:
08:00 pm June 3, 2012 - 07:59 pm June 4, 2012
(DOY 156/0000z - 156/2359z)
Significant Spacecraft Anomalies: (The following are preliminary reports of potential non-nominal performance that will be investigated.) HSTARs: none COMPLETED OPS REQUEST: 19263-0 - Clear COS Event Flag 3 for prop 12810 visits 18-19@156/1802z COMPLETED OPS NOTES: none FGS ACQ STATUS: SCHEDULED SUCCESSFUL FGS GSAcq 7 7 FGS REAcq 9 9 OBAD with Maneuver 6 6 SIGNIFICANT EVENTS: The COS FUV Special Recovery activities (proposal 12810 visits 16 - 17) successfully completed today without incident. The FUV was ramped to the 2nd HV plateau (-5010V/-4963V (160/157)) similar to visit 10; however this time the QE grid was on, no elevated counts or HV current transients were observed in the engineering telemetry during or after the ramp. The STScI and MOSES2 Engineering Teams have examined the relevant telemetry and confirmed all voltages, currents and temperatures were as expected. The voltage and current monitors matched the signatures seen in SMOV. The COS Science Team at STScI has examined the science data and DCE memory dumps and everything is nominal. No HV current transients or unexpected elevated count rates were observed in the DCE memory dumps. The science data consisted of 2 sets of dark and wavecal exposures. The exposures were collected immediately after ramping to HVNom (160/157) and an hour later at the same HV level. Comparisons with SMOV data indicates comparable behavior when the aging of the detector and temporal fluctuations are considered. The Engineering and Science Teams have given a "Go" to proceed with visit 18 and 19. Visits 18 and 19 are scheduled for Tuesday June 5 (DOY 157). The COS event flag 3 was cleared @156/18:02 via OR 19263 -jb
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
12461 | Adam Riess, The Johns Hopkins University | Supernova Follow-up for MCT |
12500 | Sugata Kaviraj, Imperial College of Science Technology and Medicine | High-resolution UV studies of SAURON galaxies with WFC3: constraining recent star formation and its drivers in local early-type galaxies |
12534 | Harry Teplitz, California Institute of Technology | The Panchromatic Hubble Ultra Deep Field: Ultraviolet Coverage |
12582 | Ariel Goobar, Stockholm University | Probing the explosion environment and origin of Type Ia supernovae |
Calibration Observations Scheduled | ||
12351 | Knox Long, Space Telescope Science Institute | IR Persistence 18 |
12689 | Tiffany Borders, Space Telescope Science Institute | WFC3 UVIS CCD Daily Monitor |
12695 | Michael Dulude, Space Telescope Science Institute | IR Dark Monitor |
12709 | Cheryl Pavlovsky, Space Telescope Science Institute | UVIS and IR Earth Flats |
12732 | David Golimowski, Space Telescope Science Institute | CCD Hot Pixel Annealing |
12742 | Justin Ely, Space Telescope Science Institute | CCD Dark Monitor Part 2 |
12744 | Justin Ely, Space Telescope Science Institute | CCD Bias and Read Noise Monitor-Part 2 |
12782 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor {Part 2} |
Other Observations Scheduled | ||
12810 | Thomas Wheeler, Space Telescope Science Institute | COS/FUV Special Recovery |