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Astrobiology|October 16, 2019
Obliquity Evolution of the Potentially Habitable Exoplanet Kepler-62fBilly Quarles, Jason W Barnes, Jack J Lissauer, et al.Astrobiology|November 16, 2019
Protein Stability in Titan's Subsurface Water OceanKyle P Martin, Shannon M MacKenzie, Jason W Barnes, et al.Astrobiology|June 22, 2016
Obliquity Variability of a Potentially Habitable Early VenusJason W Barnes, Billy Quarles, Jack J Lissauer, et al.Applied Immunohistochemistry & Molecular Morphology : AIMM|February 28, 2008
Markers of epithelial-mesenchymal transition and epithelial differentiation in sarcomatoid carcinoma: utility in the differential diagnosis with sarcomaJustin M M Cates, William D Dupont, Jason W Barnes, et al.Astrobiology|May 3, 2018
Strategies for Detecting Biological Molecules on TitanCatherine D Neish, Ralph D Lorenz, Elizabeth P Turtle, et al.Planetary Science|August 12, 2016
<i>Cassini</i>/VIMS observes rough surfaces on Titan's Punga Mare in specular reflectionJason W Barnes, Christophe Sotin, Jason M Soderblom, et al.Nature|June 5, 2009
Global circulation as the main source of cloud activity on TitanSébastien Rodriguez, Stéphane Le Mouélic, Pascal Rannou, et al.Science (New York, N.Y.)|March 11, 2006
Composition and physical properties of Enceladus' surfaceRobert H Brown, Roger N Clark, Bonnie J Buratti, et al.Science (New York, N.Y.)|October 8, 2005
A 5-micron-bright spot on Titan: evidence for surface diversityJason W Barnes, Robert H Brown, Elizabeth P Turtle, et al.Pageof 1