Earlier reports | Convert Day of Year |
Daily Report #8479
Period Covered:
08:00 PM September 30, 2019 - 07:59 PM October 01, 2019
(DOY 274/0000z - 274/2359z)
Program | Principal Investigator | Program Title |
---|---|---|
Science Observations Scheduled | ||
15070 | Kevin France, University of Colorado at Boulder | An HST Spectroscopic Study of Protoplanetary Disk Abundances: CO/H2 Conversion Factors and Absolute Abundances for JWST |
15073 | Boris Gaensicke, The University of Warwick | Extreme evolved solar systems (EESS) |
15333 | Ian Crossfield, University of Kansas Center for Research, Inc. | The Atmospheric Diversity of Mini-Neptunes in Multi-planet Systems |
15445 | William Keel, University of Alabama | Gems of the Galaxy Zoos |
15655 | Sean Johnson, Princeton University | The first high resolution view of the full extent, morphology, and multi-phase nature of radio-loud and quiet AGN feedback with ACS+SBC |
15659 | Douglas Gies, Georgia State University Research Foundation | The Missing Link in Massive Binary Star Evolution |
15660 | Christopher Johns-Krull, Rice University | Testing M Dwarf Mass Loss Across the Fully Convective Boundary |
15661 | Michael McDonald, Massachusetts Institute of Technology | Testing the Limits of AGN Feedback in Starburst and QSO Central Cluster Galaxies |
Calibration Observations Scheduled | ||
15533 | Camellia Magness, Space Telescope Science Institute | COS/FUV Detector Dark Monitor |
15534 | David Sahnow, Space Telescope Science Institute | Cycle 26 COS FUV Detector Gain Maps |
15548 | Doug Branton, Space Telescope Science Institute | STIS CCD Dark Monitor Part 3 |
15550 | Doug Branton, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 2 |
15568 | Heather Kurtz, Space Telescope Science Institute | UVIS Bowtie Monitor |
15571 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS Daily Monitor C |
15592 | Ben Sunnquist, Space Telescope Science Institute | WFC3 CSM monitor with earth flats |
15724 | Marc Rafelski, Space Telescope Science Institute | WFC3 IR Linearity Monitor |