Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
17308 |
Cameron Lemon, Stockholm University |
An HST Gap Program for lensed Quasars |
17502 |
David Thilker, The Johns Hopkins University |
Resolving gas, star formation and feedback in nearby galaxies with an HST+JWST+ALMA Treasury |
17770 |
Daichi Hiramatsu, Harvard University |
Unveiling the Progenitors of Interacting Supernovae with Resolved Host Galaxy Imaging in the Rest-Frame UV |
17776 |
Sean Terry, University of Maryland |
A Precursor Survey of the Roman Galactic Bulge Time Domain Fields |
17793 |
Brian Wood, Naval Research Laboratory |
Stellar Rotation and Winds for Old Sun-like Stars |
17803 |
Sean Johnson, University of Michigan |
The first multi-phase survey of the circumgalactic medium of quasar hosts at z<1 |
17804 |
R. O. Loyd, Eureka Scientific Inc. |
STELa: Survey of Transiting Exoplanets in Lyman-alpha |
17815 |
Alexander Beckett, Space Telescope Science Institute |
DISCS: Direct Imaging Survey of Circumgalactic Structure |
17927 |
Ashley Chrimes, European Space Agency - ESTEC |
Unveiling the origin of magnetars through a large proper motion sample |
Calibration Observations Scheduled |
17630 |
Matthew Dallas, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 2 |
17633 |
Joshua Lothringer, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 2 |
17635 |
Matthew Dallas, Space Telescope Science Institute |
STIS CCD Spectroscopic Flats |
17666 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS Bowtie Monitor |
17668 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 2 |
17675 |
Anne O'Connor, Space Telescope Science Institute |
WFC3 Characterization of UVIS Traps with Charge Injection |
17677 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 IR Dark Monitor |
17692 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |
17931 |
Jay Anderson, Space Telescope Science Institute |
Enhanced Pixel-based CTE Model Internal Observations |