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Daily Report #7185
Period Covered:
08:00 pm March 15, 2016 - 07:59 pm March 16, 2016
(DOY 076/0000z - 076/2359z)
This report was generated by the HST Automated Report System @2016-03-17 17:02:00 GMT
Significant Spacecraft Anomalies: (The following are preliminary reports of potential non-nominal performance that will be investigated.)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 14071 | Sanchayeeta Borthakur, The Johns Hopkins University | How are HI Disks Fed? Probing Condensation at the Disk-Halo Interface |
| 14077 | Boris Gaensicke, The University of Warwick | The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps |
| 14141 | Guy Worthey, Washington State University | NGSL Extension 1. Hot Stars and Evolved Stars |
| 14254 | Tommaso Treu, University of California - Los Angeles | Accurate cosmography from gravitational time delays: 2.3% on H0 from deep WFC3 images of lensed quasars |
| 14327 | Saul Perlmutter, University of California - Berkeley | See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts |
| 14469 | Carlo Manara, European Space Agency - ESTEC | The HST-ALMA connection: measuring the FUV spectrum of a newly discovered transition disk down to the H2 and CO photodissociation regime |
| Calibration Observations Scheduled | ||
| 14369 | Matthew Bourque, Space Telescope Science Institute | WFC3 UVIS Daily Monitor B |
| 14381 | Knox Long, Eureka Scientific Inc. | WFC3 IR Persistence: Position Dependent Model |
| 14382 | Sylvia Baggett, Space Telescope Science Institute | WFC3/UVIS contamination and stability monitor |
| 14389 | Heather Gunning, Space Telescope Science Institute | WFC3 UVIS Pixel variations via int-flat monitor |
| 14396 | David Golimowski, Space Telescope Science Institute | CCD Daily Monitor (Part 2) |
| 14412 | Joanna Taylor, Space Telescope Science Institute | CCD Dark Monitor Part 1 |
| 14414 | Joanna Taylor, Space Telescope Science Institute | CCD Bias and Read Noise Monitor Part 2 |
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