Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
12466 |
Jane Charlton, The Pennsylvania State University |
The State of High Ionization Gas in 11 Intermediate Redshift Galaxies and Their Surroundings |
12488 |
Mattia Negrello, Open University |
SNAPshot observations of gravitational lens systems discovered via wide-field Herschel imaging |
12539 |
Nils Bergvall, Uppsala Astronomical Observatory |
A novel approach to find Lyman continuum leaking galaxies at z~0.3 with COS |
12568 |
Matthew Malkan, University of California - Los Angeles |
WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time |
12870 |
Boris Gaensicke, The University of Warwick |
The mass and temperature distribution of accreting white dwarfs |
12903 |
Luis Ho, Carnegie Institution of Washington |
The Evolutionary Link Between Type 2 and Type 1 Quasars |
Calibration Observations Scheduled |
13072 |
Matthew Bourque, Space Telescope Science Institute |
UVIS Bowtie Monitor |
13074 |
John Biretta, Space Telescope Science Institute |
UVIS CCD Daily Monitor B |
13084 |
Elena Sabbi, Space Telescope Science Institute - ESA |
Characterization of UVIS Traps with CI |
13085 |
Sylvia Baggett, Space Telescope Science Institute |
Line10 Charge Injection Biases |
13086 |
Knox Long, Space Telescope Science Institute |
WFC3 IR Persistance as a Function of Saturation Time |
13089 |
Susana Deustua, Space Telescope Science Institute |
WFC3 UVIS & IR Photometry |
13093 |
Janice Lee, Space Telescope Science Institute |
IR Grisms: Wavelength Calibration Monitor |
13099 |
Peter McCullough, Space Telescope Science Institute |
IR Earth Flats |
13131 |
Svea Hernandez, Space Telescope Science Institute |
CCD Dark Monitor Part 1 |
13133 |
Svea Hernandez, Space Telescope Science Institute |
CCD Bias and Read Noise Monitor Part 1 |
13152 |
David Golimowski, Space Telescope Science Institute |
CCD Daily Monitor {Part 1} |
13169 |
Heather Gunning, Space Telescope Science Institute |
CCD Anomalous QE Pixels |