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Daily Report #7168
Period Covered:
07:00 pm February 27, 2016 - 06:59 pm February 28, 2016
(DOY 059/0000z - 059/2359z)
This report was generated by the HST Automated Report System @2016-02-29 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 | ||
| 13646 | Ryan Foley, University of Illinois at Urbana - Champaign | Understanding the Progenitor Systems, Explosion Mechanisms, and Cosmological Utility of Type Ia Supernovae |
| 13728 | Steven Kraemer, Catholic University of America | Do QSO2s have Narrow Line Region Outflows? Implications for quasar-mode feedback |
| 14068 | Robert Barrows, University of Colorado at Boulder | Resolving the Nuclear Regions of Confirmed Offset AGN |
| 14127 | Michele Fumagalli, Durham Univ. | First Measurement of the Small Scale Structure of Circumgalactic Gas via Grism Spectra of Close Quasar Pairs |
| 14163 | Mickael Rigault, Humboldt Universitat zu Berlin | Honing Type Ia Supernovae as Distance Indicators, Exploiting Environmental Bias for H0 and w. |
| 14201 | Sangeeta Malhotra, Arizona State University | Lyman alpha escape in Green Pea galaxies (give peas a chance) |
| 14327 | Saul Perlmutter, University of California - Berkeley | See Change: Testing time-varying dark energy with z>1 supernovae and their massive cluster hosts |
| Calibration Observations Scheduled | ||
| 14367 | Meredith Durbin, Space Telescope Science Institute | UVIS Bowtie Monitor |
| 14368 | Matthew Bourque, Space Telescope Science Institute | WFC3 UVIS Daily Monitor A |
| 14385 | Norbert Pirzkal, Space Telescope Science Institute | WFC3 IR Grisms: Wavelength Calibration |
| 14389 | Heather Gunning, Space Telescope Science Institute | WFC3 UVIS Pixel variations via int-flat monitor |
| 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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