K. Harshman

TL;DR: Higher abundances of chlorinated hydrocarbons in the mudstone compared with Rocknest windblown materials previously analyzed by Curiosity suggest that indigenous martian or meteoritic organic carbon sources may be preserved in the Mudstone; however, the carbon source for the chlorinatedHydrocarbons is not definitively of martian origin.

TL;DR: The Mars Odyssey Gamma-Ray Spectrometer (MOGRS) is a suite of three different instruments, a gamma subsystem (GS), a neutron spectrometer, and a high-energy neutron detector, working together to collect data that will permit the mapping of elemental concentrations on the surface of Mars.

TL;DR: The LCROSS impact site inside the Cabeus crater demonstrates the highest hydrogen concentration in the lunar south polar region, corresponding to an estimated content of 0.5 to 4.0% water ice by weight, depending on the thickness of any overlying dry regolith layer.

TL;DR: In this paper, a generalized analytic formalism for the inverse Compton X-ray emission from hydrogen-poor supernovae is presented and applied to SN 2011fe using Swift X-Ray Telescope (XRT), UVOT, and Chandra observations.

TL;DR: The OSIRIS-REx Camera Suite (OCAMS) as discussed by the authors consists of three cameras, the MapCam, the SamCam and the PolyCam, which are used to collect color images of the surface of the asteroid Bennu.