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Daily Report #6492
Period Covered:
08:00 pm April 22, 2014 - 07:59 pm April 23, 2014
(DOY 113/0000z - 113/2359z)
This report was generated by the HST Automated Report System @2014-04-24 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 7 7 OBAD with Maneuver 7 7 SIGNIFICANT EVENTS: none
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
13303 | Robert Simcoe, Massachusetts Institute of Technology | The Structure of MgII Absorbing Galaxies at z=2-5: Linking CGM Physics and Stellar Morphology During Galaxy Assembly |
13312 | Danielle Berg, University of Minnesota - Twin Cities | The Evolution of C/O in Low Metallicity Dwarf Galaxies |
13330 | Bradley Peterson, The Ohio State University | Mapping the AGN Broad Line Region by Reverberation |
13364 | Daniela Calzetti, University of Massachusetts - Amherst | LEGUS: Legacy ExtraGalactic UV Survey |
13366 | Roelof de Jong, Leibniz-Institut fur Astrophysik Potsdam (AIP) | The vertical disk structure of spiral galaxies and the origin of their thick disks |
13376 | Kristen McQuinn, University of Minnesota - Twin Cities | The Star Formation History of Leo P |
13467 | Jacob Bean, University of Chicago | Follow The Water: The Ultimate WFC3 Exoplanet Atmosphere Survey |
Calibration Observations Scheduled | ||
13518 | Svea Hernandez, Space Telescope Science Institute | CCD Dark Monitor Part 1 |
13535 | Svea Hernandez, Space Telescope Science Institute | CCD Bias and Read Noise Monitor Part 1 |
13554 | Sylvia Baggett, Space Telescope Science Institute | WFC3 UVIS Anneal |
13588 | Peter McCullough, Space Telescope Science Institute | CSM monitor with earth flats |
13590 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor {Part 2} |
13624 | Elena Sabbi, Space Telescope Science Institute | Monitoring Persistence in WFC3/IR after scanned grism observations |
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