| Earlier reports | Convert Day of Year |
Daily Report #6639
Period Covered:
08:00 pm September 16, 2014 - 07:59 pm September 17, 2014
(DOY 260/0000z - 260/2359z)
This report was generated by the HST Automated Report System @2014-09-18 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 7 7 FGS REAcq 8 8 OBAD with Maneuver 6 6 SIGNIFICANT EVENTS: none
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 13335 | Adam Riess, The Johns Hopkins University | HST and Gaia, Light and Distance |
| 13364 | Daniela Calzetti, University of Massachusetts - Amherst | LEGUS: Legacy ExtraGalactic UV Survey |
| 13377 | Andrea Mehner, European Southern Observatory - Chile | Essential UV Observations of Eta Carinae's Change of State |
| 13441 | Rachael Tomasino, University of Denver | Co-latitudinal Radial Veloctiy Profile Confirmation Via Differential Proper Motion of the Bipolar Egg Nebula |
| 13691 | Wendy Freedman, Carnegie Institution of Washington | CHP-II: The Carnegie Hubble Program to Measure Ho to 3% Using Population II |
| 13739 | Evan Skillman, University of Minnesota - Twin Cities | Is the First Epoch of Star Formation in Satellite Galaxies Universal? - Part II |
| 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 |
| 13558 | Matthew Bourque, Space Telescope Science Institute | UVIS CCD Daily Monitor C |
| 13591 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor {Part 3} |
| 13615 | Colin Cox, Space Telescope Science Institute | HST Cycle 21 Focus and Optical Monitor |
| 13624 | Elena Sabbi, Space Telescope Science Institute | Monitoring Persistence in WFC3/IR after scanned grism observations |
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