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Joseph Twicken Jon M, Jenkins Shawn E, Seader Peter Tenenbaum Jeffrey Smith Lee S, Brownston Christopher Burke Joseph Catanzarite Bruce Clarke Miles T, Cote
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Published in
arXiv preprint arXiv:1604.06140
We present results of the final Kepler Data Processing Pipeline search for transiting planet signals in the full 17-quarter primary mission dataset. The search includes a total of 198,709 stellar targets of which 112,046 were observed in all 17 quarters and 86,663 in fewer than 17 quarters. We report on 17,230 targets for which at least one transit...
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Jeffrey Smith Jason H, Steffen Martin, Still Peter Tenenbaum Susan E, Thompson Joseph Twicken Christa, Van Laerhoven Angie, Wolfgang Khadeejah A, Zamudio Jason Rowe
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Published in
The Astrophysical Journal Supplement Series
The Kepler mission discovered 2842 exoplanet candidates with 2 yr of data. We provide updates to the Kepler planet candidate sample based upon 3 yr (Q1? Q12) of data. Through a series of tests to exclude false-positives, primarily caused by eclipsing binary stars and instrumental systematics, 855 additional planetary candidates have been discovered...
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Daniel C, Fabrycky Jack J, Lissauer Darin, Ragozzine Jason Rowe Jason H, Steffen Eric, Agol Thomas, Barclay Natalie, Batalha William, Borucki David R, Ciardi
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Published in
The Astrophysical Journal
We report on the orbital architectures of Kepler systems having multiple-planet candidates identified in the analysis of data from the first six quarters of Kepler data and reported by Batalha et al.(2013). These data show 899 transiting planet candidates in 365 multiple-planet systems and provide a powerful means to study the statistical propertie...
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Steve B, Howell David R, Ciardi Brice-Olivier, Demory Douglas Caldwell William J, Borucki Jessie L, Christiansen Jon M, Jenkins Todd C, Klaus Benjamin J, Fulton Robert Morris
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Published in
The Astrophysical Journal
We present high precision photometry of Kepler-41, a giant planet in a 1.86 day orbit around a G6V star that was recently confirmed through radial velocity measurements. We have developed a new method to confirm giant planets solely from the photometric light curve, and we apply this method herein to Kepler-41 to establish the validity of this tech...
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Susan E, Thompson Thomas, Barclay Jason Rowe Jack J, Lissauer Daniel Huber Franois, Fressin Steve B, Howell Stephen T, Bryson William J, Chaplin Jean-Michel, Desert
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Published in
Nature
Since the discovery of the first exoplanets1,2, it has been known that other planetary systems can look quite unlike our own3. Until fairly recently, we have been able to probe only the upper range of the planet size distribution4,5, and, since last year, to detect planets that are the size of Earth6 or somewhat smaller7. Hitherto, no planets have ...
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G, Torres D G, Koch Joseph Twicken J J, Lissauer K, Uddin W, Rapin Jeffrey Van Cleve G S, Basri L, Walkowicz A P, Boss
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Published in
VizieR Online Data Catalog
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Jeffrey Smith Martin C. Stumpe Jeffrey Van Cleve Jon M. Jenkins Thomas S. Barclay Michael N. Fanelli Forrest R. Girouard Jeffery J. Kolodziejczak Sean D. McCauliff Robert Morris
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Published in
arXiv preprint arXiv:1602.03204
With the unprecedented photometric precision of the Kepler spacecraft, significant systematic and stochastic errors on transit signal levels are observable in the Kepler photometric data. These errors, which include discontinuities, outliers, systematic trends, and other instrumental signatures, obscure astrophysical signals. The presearch data con...
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Robert Morris Christopher K, Middour Fergal Mullally Samuel N, Quinn Elisa Quintana Avi, Shporer Martin, Still Peter Tenenbaum Susan E, Thompson Joseph Twicken
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Published in
Monthly Notices of the Royal Astronomical Society
We present a method to confirm the planetary nature of objects in systems with multiple transiting exoplanet candidates. This method involves a Fourier-domain analysis of the deviations in the transit times from a constant period that result from dynamical interactions within the system. The combination of observed anticorrelations in the transit t...
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Sandra M., Wiseman R. E., Arvidson Robert Morris F., Poulet J. C., Andrews-Hanna Janice Bishop S. L., Murchie F. P., Seelos D., Des Marais J. L., Griffes
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Published in
Journal of Geophysical Research Space Physics
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Kimberly A., Lichtenberg Raymond E., Arvidson Robert Morris Scott L., Murchie Janice Bishop David, Fernandez Remolar Timothy D., Glotch Eldar, Noe Dobrea John F., Mustard Jeffrey, Andrews-Hanna
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Published in
Journal of Geophysical Research Space Physics
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Nathalie Cabrol Edmond Grin Guillermo, Chong Edwin, Minkley Andrew N, Hock Youngseob, Yu Leslie, Bebout Erich, Fleming Donat P, Haeder Cecilia, Demergasso
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Published in
Journal of Geophysical Research Biogeosciences
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Scott, Murchie Leah, Roach Frank, Seelos Ralph, Milliken John, Mustard Raymond, Arvidson Sandra, Wiseman Kimberly, Lichtenberg Jeffrey, Andrews-Hanna Janice Bishop
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Published in
Journal of Geophysical Research Space Physics
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Mariek E, Schmidt Steven W, Ruff Timothy J, Mccoy William H, Farrand Jeffrey R, Johnson Ralf, Gellert Douglas W, Ming Robert Morris Nathalie Cabrol Kevin W, Lewis
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Published in
Journal of Geophysical Research: Planets
[1] In the Inner Basin of the Columbia Hills, Gusev Crater is Home Plate, an 80 m platform of layered clastic rocks of the Barnhill class with microscopic and macroscopic textures, including a bomb sag, suggestive of a phreatomagmatic origin. We present data acquired by the Spirit Mars Exploration Rover by Alpha Particle X-Ray Spectrometer (APXS), ...
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S., Murchie R., Arvidson P., Bedini K., Beisser J.-P., Bibring Janice Bishop J., Boldt P., Cavender T., Choo R. T., Clancy
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Published in
Journal of Geophysical Research Space Physics
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H Y, Mcsween S W, Ruff Robert Morris J F, Bell K, Herkenhoff Ralf, Gellert K R, Stockstill Livio Leonardo Tornabene S W, Squyres J A, Crisp
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Published in
Journal of Geophysical Research: Planets
[1] Irvine, Backstay, and Wishstone are the type specimens for three classes of fine- grained or fragmental, relatively unaltered rocks with distinctive thermal emission spectra, found as float on the flanks of the Columbia Hills. Chemical analyses indicate that these rocks are mildly alkaline basalt, trachybasalt, and tephrite, respectively. Their...
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J F, Bell S W, Squyres R E, Arvidson H M, Arneson D, Bass D, Blaney Nathalie Cabrol W, Calvin J, Farmer W H, Farrand
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Published in
Science
Panoramic Camera images at Gusev crater reveal a rock-strewn surface interspersed with high-to moderate-albedo fine-grained deposits occurring in part as drifts or in small circular swales or hollows. Optically thick coatings of fine-grained ferric iron–rich dust dominate most bright soil and rock surfaces. Spectra of some darker rock surfaces and ...
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K E, Herkenhoff S W, Squyres J F, Bell J N, Maki H M, Arneson P, Bertelsen D I, Brown S A, Collins A, Dingizian S T, Elliott
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Published in
Journal of Geophysical Research: Planets
[1] The Athena science payload on the Mars Exploration Rovers (MER) includes the Microscopic Imager (MI). The MI is a fixed-focus camera mounted on the end of an extendable instrument arm, the Instrument Deployment Device (IDD). The MI was designed to acquire images at a spatial resolution of 30 microns/pixel over a broad spectral range (400–700 nm...
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Virginia Gulick Robert Morris Mark A, Ruzon Ted L, Roush
Published in
Journal of Geophysical Research: Planets
A Martian rover capable of analyzing images autonomously could traverse greater path lengths and return data with greater scientific content. A more intelligent rover could, for example, automatically select targets of interest (eg, rocks, layers), return spectral or high- resolution image data of these targets at the same time, remove less interes...
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Robert Morris D C, Golden James F, Bell Tad D, Shelfer Andreas C, Scheinost Nancy W, Hinman George, Furniss Stanley A, Mertzman Janice Bishop Douglas W, Ming
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Published in
Journal of Geophysical Research: Planets
Major element, multispectral, and magnetic properties data were obtained at Ares Vallis during the Mars Pathfinder mission. To understand the compositional, mineralogical, and process implications of these data, we obtained major element, mineralogical, and magnetic data for well-crystalline and nanophase ferric minerals, terrestrial analogue sampl...
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S, Murchie O, Barnouin-Jha K, Barnouin-Jha Janice Bishop J, Johnson H, Mcsween Robert Morris
