| Earlier reports | Convert Day of Year |
Daily Report #8160
Period Covered:
07:00 PM November 15, 2018 - 06:59 PM November 16, 2018
(DOY 320/0000z - 320/2359z)
| Program | Principal Investigator | Program Title |
|---|---|---|
| Science Observations Scheduled | ||
| 15075 | Jay Howk, University of Notre Dame | The CGM of Massive Galaxies: Where Cold Gas Goes to Die? |
| 15156 | Yong Zheng, University of California - Berkeley | Mapping Gas Flows from the Disk to the Circumgalactic Medium |
| 15215 | Vardha Bennert, Cal Poly Corporation, Sponsored Programs Department | A Local Baseline of the Black Hole Mass - Host Galaxy Scaling Relations for Active Galaxies |
| 15253 | Raoul Canameras, University of Copenhagen, Niels Bohr Institute | The nature of ultra-massive lens galaxies |
| 15307 | Michael Gladders, University of Chicago | Building the SPT-HST Legacy: Imaging Massive Clusters to z=1.5 |
| 15340 | Timothy Heckman, The Johns Hopkins University | The HST-pNFL program: Mapping the Fluorescent Emission of Galactic Outflows |
| 15361 | Robert Fesen, Dartmouth College | The Mysterious High-Velocity Ejecta Jets in Cassiopeia A |
| 15363 | Nao Suzuki, Institute for Physics and Mathematics of the Universe | SUbaru Supernovae with Hubble Infrared (SUSHI) |
| 15502 | Amy Simon, NASA Goddard Space Flight Center | Hubble 2020: Outer Planet Atmospheres Legacy (OPAL) Program |
| Calibration Observations Scheduled | ||
| 15519 | Tyler Desjardins, Space Telescope Science Institute | CCD Daily Monitor (Part 1) |
| 15533 | Camellia Magness, Space Telescope Science Institute | COS/FUV Detector Dark Monitor |
| 15546 | Doug Branton, Space Telescope Science Institute | STIS CCD Dark Monitor Part 1 |
| 15549 | Doug Branton, Space Telescope Science Institute | STIS CCD Bias and Read Noise Monitor Part 1 |
| 15563 | Sean Lockwood, Space Telescope Science Institute | STIS NUV MAMA Dark Monitor |
| 15569 | Catherine Martlin, Space Telescope Science Institute | WFC3 UVIS Daily Monitor A |
| 15589 | Clare Shanahan, Space Telescope Science Institute | WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |
| 15592 | Ben Sunnquist, Space Telescope Science Institute | WFC3 CSM monitor with earth flats |
Forward this Message to a Friend »
Subscription Reminder: You're Subscribed to: [HST REPORTS] using the address: example@example.com
From:
list.admin@aus-city.com
https://aus-city.com