| Program |
Principal Investigator |
Program Title |
| Science Observations Scheduled |
| 17455 |
Yue Shen, University of Illinois at Urbana - Champaign |
A Snapshot Survey of Sub-arcsec Dual Quasars and Lenses at z>2 |
| 17513 |
Paul Bennet, Space Telescope Science Institute |
Proper Motions of Galaxies in the M81 Group: Unleashing the Full Power of HST's 20-year Time Baseline |
| 17697 |
Matti Dorsch, Universitat Potsdam |
A far-UV treasury survey for hot subdwarf stars |
| 17734 |
Bart Wakker, Eureka Scientific Inc. |
A clean view of the CGM for well-characterized galaxies |
| 17769 |
George Pavlov, The Pennsylvania State University |
The UVOIR portrait of PSR J0030+0451, the key millisecond pulsar |
| 17796 |
Stefano Valenti, University of California - Davis |
Tracing the mass-loss history from type II supernova explosions back through the red supergaint phase. |
| 17797 |
Eric Bell, University of Michigan |
Galactic Underdogs: Assessing the True Satellite Galaxy Population in the Local Volume |
| 17804 |
R. O. Loyd, Eureka Scientific Inc. |
STELa: Survey of Transiting Exoplanets in Lyman-alpha |
| 17819 |
Laura Rogers, NOIRLab - (AZ) |
WD0106-038: the first variable metal polluted white dwarf? |
| Calibration Observations Scheduled |
| 17631 |
Matthew Dallas, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 3 |
| 17633 |
Joshua Lothringer, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 2 |
| 17655 |
Alyssa Guzman, Space Telescope Science Institute |
CCD Daily Monitor (Part 3) |
| 17669 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 3 |
| 17689 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 UVIS Pixel-to-Pixel QE Variations via Internal Flats |
| 17692 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |
| 17906 |
Annalisa Calamida, Space Telescope Science Institute |
HST/WFC3 Observations for Cross-Mission Flux Calibration |
| 17942 |
Sten Hasselquist, Space Telescope Science Institute |
COS FUV LP10 Calibration: Supplemental Profiles and Traces |