Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
17069 |
Matthew Hayes, Stockholm University |
The Lyman-alpha and Continuum Origins Survey (LaCOS) |
17310 |
Michael Koss, Eureka Scientific Inc. |
A Blue Gap Survey of Nearby Active Galaxies |
17420 |
Boris Gaensicke, The University of Warwick |
A legacy survey for evolved planetary systems within 100pc |
17464 |
Adam Kowalski, University of Colorado at Boulder |
From High-Energy Particle Beam Heating in Stars to Ozone Destruction in Planets: NUV Spectra as the Fulcrum for a Comprehensive Understanding of Flaring M Dwarf Systems |
17483 |
Rajeshwari Dutta, Inter-University Centre for Astronomy and Astrophysics |
Characterizing Lyman-Alpha emitters with Snapshot Survey (CLASS) |
17487 |
Yasaman Homayouni, The Pennsylvania State University |
A Fundamental Test of Black Hole Masses: Ultraviolet Echo Mapping the Multi-Scale Broad Line Gas around Quasars |
17492 |
Brendan O'Connor, Carnegie Mellon University |
Zooming in on the locations of short gamma-ray bursts |
17504 |
Patrick Kelly, University of Minnesota - Twin Cities |
SNAP Survey for Strongly Lensed Supernovae and Magnified Stars |
Calibration Observations Scheduled |
17346 |
Harish Khandrika, Space Telescope Science Institute |
WFC3 UVIS Bowtie Monitor |
17347 |
Aidan Pidgeon, Space Telescope Science Institute |
WFC3 UVIS CCD Daily Monitor Part 1 |
17361 |
Annalisa Calamida, Space Telescope Science Institute |
WFC3 UVIS and IR Photometry |
17371 |
Frederick Dauphin, Space Telescope Science Institute |
WFC3 CSM Monitor with Earth Flats |
17374 |
Sophia Medallon, Space Telescope Science Institute |
STIS CCD Dark Monitor Part 1 |
17377 |
Daniel Stapleton, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 1 |
17380 |
Matthew Dallas, Space Telescope Science Institute |
STIS CCD Spectroscopic Flats |
17391 |
Amy Jones, Space Telescope Science Institute |
STIS NUV MAMA Dark Monitor |
17586 |
Debopam Som, Space Telescope Science Institute |
WFC3 IR Time-Dependent Sensitivity: Spatial Scans |