Program |
Principal Investigator |
Program Title |
Science Observations Scheduled |
13283 |
Xinyu Dai, University of Oklahoma Norman Campus |
Testing ISM Evolution Models with Gravitational Lenses |
13313 |
Mederic Boquien, University of Cambridge |
Determining attenuation laws down to the Lyman break in z~0.3 galaxies |
13330 |
Bradley Peterson, The Ohio State University |
Mapping the AGN Broad Line Region by Reverberation |
13334 |
Adam Riess, The Johns Hopkins University |
The Longest Period Cepheids, a bridge to the Hubble Constant |
13344 |
Adam Riess, The Johns Hopkins University |
A 1% Measurement of the Distance Scale with Perpendicular Spatial Scanning |
13423 |
Ryan Cooke, University of California - Santa Cruz |
Primordial lithium in z~0, metal-poor damped Lyman alpha systems |
13443 |
Roeland van der Marel, Space Telescope Science Institute |
Proper Motions along the Orphan Stream: Finding the Parent, Orbit, and Milky Way Halo Shape |
13517 |
Matthew Malkan, University of California - Los Angeles |
WFC3 Infrared Spectroscopic Parallel Survey WISP: A Survey of Star Formation Across Cosmic Time |
Calibration Observations Scheduled |
13518 |
Svea Hernandez, Space Telescope Science Institute |
CCD Dark Monitor Part 1 |
13527 |
Azalee Bostroem, Space Telescope Science Institute |
NUV Spectroscopic Sensitivity Monitoring |
13535 |
Svea Hernandez, Space Telescope Science Institute |
CCD Bias and Read Noise Monitor Part 1 |
13544 |
Hugues Sana, Space Telescope Science Institute - ESA |
STIS/CCD Spectroscopic Sensitivity Monitor for Cycle 21 |
13548 |
Hugues Sana, Space Telescope Science Institute - ESA |
MAMA Spectroscopic Sensitivity and Focus Monitor Cycle 21 |
13557 |
Matthew Bourque, Space Telescope Science Institute |
UVIS CCD Daily Monitor B |
13588 |
Peter McCullough, Space Telescope Science Institute |
CSM monitor with earth flats |
13590 |
David Golimowski, Space Telescope Science Institute |
CCD Daily Monitor {Part 2} |
13624 |
Elena Sabbi, Space Telescope Science Institute |
Monitoring Persistence in WFC3/IR after scanned grism observations |