J
Josh Carter
Researcher at Massachusetts Institute of Technology
Publications - 2
Citations - 322
Josh Carter is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Kepler-22b & Circumbinary planet. The author has an hindex of 2, co-authored 2 publications receiving 318 citations.
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Journal ArticleDOI
Kepler-22b: a 2.4 Earth-radius Planet in the Habitable Zone of a Sun-like Star
William J. Borucki,David G. Koch,Natalie M. Batalha,Stephen T. Bryson,Jason F. Rowe,Francois Fressin,Guillermo Torres,Douglas A. Caldwell,Jørgen Christensen-Dalsgaard,Jørgen Christensen-Dalsgaard,William D. Cochran,Edna DeVore,Thomas N. Gautier,John C. Geary,Ronald L. Gilliland,Alan Gould,Steve B. Howell,Jon M. Jenkins,David W. Latham,Jack J. Lissauer,Geoffrey W. Marcy,Dimitar Sasselov,Alan P. Boss,David Charbonneau,David R. Ciardi,Lisa Kaltenegger,Laurance R. Doyle,Andrea K. Dupree,Eric B. Ford,Jonathan J. Fortney,Matthew J. Holman,Jason H. Steffen,Fergal Mullally,Martin Still,Jill Tarter,Sarah Ballard,Lars A. Buchhave,Josh Carter,Jessie L. Christiansen,Brice-Olivier Demory,Jean-Michel Desert,Courtney D. Dressing,Michael Endl,Daniel C. Fabrycky,Debra A. Fischer,Michael R. Haas,Christopher E. Henze,Elliott P. Horch,Andrew W. Howard,Howard Isaacson,Hans Kjeldsen,John Asher Johnson,Todd C. Klaus,Jeffery J. Kolodziejczak,Thomas Barclay,Jie Li,Søren Meibom,Andrej Prsa,Samuel N. Quinn,Elisa V. Quintana,Paul Robertson,William Sherry,Avi Shporer,Peter Tenenbaum,Susan E. Thompson,Joseph D. Twicken,Jeffrey Van Cleve,William F. Welsh,Sarbani Basu,William J. Chaplin,Andrea Miglio,Steven D. Kawaler,Torben Arentoft,Dennis Stello,Travis S. Metcalfe,Graham A. Verner,Christoffer Karoff,Mia S. Lundkvist,Mikkel N. Lund,Rasmus Handberg,Yvonne Elsworth,Saskia Hekker,Saskia Hekker,Daniel Huber,Daniel Huber,Timothy R. Bedding,William Rapin +86 more
TL;DR: A search of the time-series photometry from NASA's Kepler spacecraft reveals a transiting planet candidate orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days as discussed by the authors.
Journal ArticleDOI
Deuterium Abundance in the Interstellar Gas of the Galactic Anticenter from the 327 MHz Line
TL;DR: The deuterium abundance in the primordial gas formed during the big bang is dependent on the baryon-to-photon ratio during nucleosynthesis as mentioned in this paper, which is measured by a 6 σ detection of the hyperfine ground-state transition of deutanium at 327 MHz (92 cm) in emission from the interstellar gas in the region of the Galactic anticenter.