Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
14127 |
Michele Fumagalli, Durham Univ. |
First Measurement of the Small Scale Structure of Circumgalactic Gas via Grism Spectra of Close Quasar Pairs |
14145 |
Hsiao-Wen Chen, University of Chicago |
Characterizing Circumgalactic Gas around Passive Galaxies |
14178 |
Matthew Malkan, University of California - Los Angeles |
WFC3 Infrared Spectroscopic Parallel Survey: The WISP Deep Fields |
14216 |
Robert Kirshner, Harvard University |
RAISIN2: Tracers of cosmic expansion with SN IA in the IR |
14456 |
Mark Brodwin, University of Missouri - Kansas City |
Determining the Role of Merging in the Growth of the Galaxy Cluster Population in the Massive and Distant Clusters of WISE Survey |
14634 |
Denis Grodent, Universite de Liege |
HST-Juno synergistic approach of Jupiter's magnetosphere and ultraviolet auroras |
14651 |
Matt Darnley, Liverpool John Moores University |
Recurrent Nova M31N 2008-12a: The surrounding 'Super-Remnant' - A signpost to Type Ia Supernova progenitors |
14734 |
Nitya Kallivayalil, The University of Virginia |
Milky Way Cosmology: Laying the Foundation for Full 6-D Dynamical Mapping of the Nearby Universe |
Calibration Observations Scheduled |
14506 |
David Golimowski, Space Telescope Science Institute |
CCD Daily Monitor (Part 1) |
14530 |
Ben Sunnquist, Space Telescope Science Institute |
UVIS Bowtie Monitor |
14531 |
Matthew Bourque, Space Telescope Science Institute |
WFC3 UVIS Daily Monitor A |
14535 |
Catherine Martlin, Space Telescope Science Institute |
UVIS post-flash monitor |
14549 |
Peter McCullough, Space Telescope Science Institute |
WFC3 CSM monitor with earth flats |
14817 |
Allyssa Riley, Space Telescope Science Institute |
CCD Dark Monitor Part 1 |
14820 |
Allyssa Riley, Space Telescope Science Institute |
STIS CCD Bias and Read Noise Monitor Part 1 |
14878 |
Peter McCullough, Space Telescope Science Institute |
WFC3 UVIS contamination using spatial scans |
14879 |
Sylvia Baggett, Space Telescope Science Institute |
WFC3/UVIS sink pixel map update |