E
Elliott P. Horch
Researcher at Southern Connecticut State University
Publications - 209
Citations - 16169
Elliott P. Horch is an academic researcher from Southern Connecticut State University. The author has contributed to research in topics: Planet & Stars. The author has an hindex of 57, co-authored 204 publications receiving 14756 citations. Previous affiliations of Elliott P. Horch include University of Massachusetts Amherst & ASTRON.
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Journal ArticleDOI
Kepler Planet-Detection Mission: Introduction and First Results
William J. Borucki,David G. Koch,Gibor Basri,Natalie M. Batalha,Timothy M. Brown,Douglas A. Caldwell,John Caldwell,Joørgen Christensen-Dalsgaard,William D. Cochran,Edna DeVore,Edward W. Dunham,Andrea K. Dupree,Thomas N. Gautier,John C. Geary,Ronald L. Gilliland,Alan Gould,Steve B. Howell,Jon M. Jenkins,Yoji Kondo,David W. Latham,Geoffrey W. Marcy,Søren Meibom,Hans Kjeldsen,Jack J. Lissauer,David G. Monet,David Morrison,Dimitar Sasselov,Jill Tarter,Alan P. Boss,Donald E. Brownlee,Toby Owen,Derek Buzasi,David Charbonneau,Laurance R. Doyle,Jonathan J. Fortney,Eric B. Ford,Matthew J. Holman,Sara Seager,Jason H. Steffen,William F. Welsh,Jason F. Rowe,Howard T. Anderson,Lars A. Buchhave,David R. Ciardi,Lucianne M. Walkowicz,W. H. Sherry,Elliott P. Horch,Howard Isaacson,Mark E. Everett,Debra A. Fischer,Guillermo Torres,John Asher Johnson,Michael Endl,Phillip J. MacQueen,Stephen T. Bryson,Jessie L. Dotson,Michael R. Haas,Jeffrey Kolodziejczak,Jeffrey Van Cleve,Hema Chandrasekaran,Joseph D. Twicken,Elisa V. Quintana,Bruce D. Clarke,Christopher C. R. Allen,Jie Li,Haley Wu,Peter Tenenbaum,E. Verner,Frederick C. Bruhweiler,Jason W. Barnes,Andrej Prsa +70 more
TL;DR: The Kepler mission was designed to determine the frequency of Earth-sized planets in and near the habitable zone of Sun-like stars, which is the region where planetary temperatures are suitable for water to exist on a planet's surface.
Journal ArticleDOI
Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data
William J. Borucki,David G. Koch,Gibor Basri,Natalie M. Batalha,Timothy M. Brown,Stephen T. Bryson,Douglas A. Caldwell,Jørgen Christensen-Dalsgaard,William D. Cochran,Edna DeVore,Edward W. Dunham,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,Jason F. Rowe,Dimitar Sasselov,Alan P. Boss,David Charbonneau,David R. Ciardi,Laurance R. Doyle,Andrea K. Dupree,Eric B. Ford,Jonathan J. Fortney,Matthew J. Holman,Sara Seager,Jason H. Steffen,Jill Tarter,William F. Welsh,Christopher C. R. Allen,Lars A. Buchhave,Jessie L. Christiansen,Bruce D. Clarke,Santanu Das,Jean-Michel Desert,Michael Endl,Daniel C. Fabrycky,Francois Fressin,Michael R. Haas,Elliott P. Horch,Andrew W. Howard,Howard Isaacson,Hans Kjeldsen,Jeffery J. Kolodziejczak,Craig Kulesa,Jie Li,Philip W. Lucas,P. Machalek,Donald W. McCarthy,Phillip J. MacQueen,Søren Meibom,Thibaut Miquel,Andrej Prsa,Samuel N. Quinn,Elisa V. Quintana,Darin Ragozzine,William Sherry,Avi Shporer,Peter Tenenbaum,Guillermo Torres,Joseph D. Twicken,Jeffrey Van Cleve,Lucianne M. Walkowicz,Fred C. Witteborn,Martin Still +69 more
TL;DR: In this article, the Kepler mission released data for 156,453 stars observed from the beginning of the science observations on 2009 May 2 through September 16, and there are 1235 planetary candidates with transit-like signatures detected in this period.
Journal ArticleDOI
Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data
William J. Borucki,David G. Koch,Gibor Basri,Natalie M. Batalha,Timothy M. Brown,Stephen T. Bryson,Douglas A. Caldwell,Jørgen Christensen-Dalsgaard,William D. Cochran,Edna DeVore,Edward W. Dunham,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,Jason F. Rowe,Dimitar Sasselov,Alan P. Boss,David Charbonneau,David R. Ciardi,Laurance R. Doyle,Andrea K. Dupree,Eric B. Ford,Jonathan J. Fortney,Matthew J. Holman,Sara Seager,Jason H. Steffen,Jill Tarter,William F. Welsh,Christopher C. R. Allen,Lars A. Buchhave,Jessie L. Christiansen,Bruce D. Clarke,Jean-Michel Desert,Michael Endl,Daniel C. Fabrycky,Francois Fressin,Michael R. Haas,Elliott P. Horch,Andrew W. Howard,Howard Isaacson,Hans Kjeldsen,Jeffery J. Kolodziejczak,Craig Kulesa,Jie Li,Pavel Machalek,Donald W. McCarthy,Phillip J. MacQueen,Søren Meibom,Thibaut Miquel,Andrej Prsa,Samuel N. Quinn,Elisa V. Quintana,Darin Ragozzine,William Sherry,Avi Shporer,Peter Tenenbaum,Guillermo Torres,Joseph D. Twicken,Jeffrey Van Cleve,Lucianne M. Walkowicz +65 more
TL;DR: In this paper, the Kepler mission released data for 156,453 stars observed from the beginning of the science observations on 2 May through 16 September 2009, and there are 1235 planetary candidates with transit-like signatures detected in this period.
Journal ArticleDOI
Characteristics of Kepler Planetary Candidates Based on the First Data Set
William J. Borucki,David G. Koch,Gibor Basri,Natalie M. Batalha,Alan P. Boss,Timothy M. Brown,Douglas A. Caldwell,Jørgen Christensen-Dalsgaard,William D. Cochran,Edna DeVore,Edward W. Dunham,Andrea K. Dupree,Thomas N. Gautier,John C. Geary,Ronald L. Gilliland,Alan Gould,Steve B. Howell,Jon M. Jenkins,Hans Kjeldsen,David W. Latham,Jack J. Lissauer,Geoffrey W. Marcy,David G. Monet,Dimitar Sasselov,Jill Tarter,David Charbonneau,Laurance R. Doyle,Eric B. Ford,Jonathan J. Fortney,Matthew J. Holman,Sara Seager,Jason H. Steffen,William F. Welsh,Christopher C. R. Allen,Stephen T. Bryson,Lars A. Buchhave,Hema Chandrasekaran,Jessie L. Christiansen,David R. Ciardi,Bruce D. Clarke,Jessie L. Dotson,Michael Endl,Debra A. Fischer,Francois Fressin,Michael R. Haas,Elliott P. Horch,Andrew W. Howard,Howard Isaacson,Jeffery J. Kolodziejczak,Jie Li,Phillip J. MacQueen,Søren Meibom,Andrej Prsa,Elisa V. Quintana,Jason F. Rowe,W. H. Sherry,Peter Tenenbaum,Guillermo Torres,Joseph D. Twicken,Jeffrey Van Cleve,Lucianne M. Walkowicz,H. Wu +61 more
TL;DR: In this paper, the identity and characteristics of 305 released stars with planetary candidates are given, and five candidates are present in and near the habitable zone; two near super-Earth size, and three bracketing the size of Jupiter.
Journal ArticleDOI
THE MASS OF KOI-94d AND A RELATION FOR PLANET RADIUS, MASS, AND INCIDENT FLUX*
Lauren M. Weiss,Geoffrey W. Marcy,Jason F. Rowe,Andrew W. Howard,Howard Isaacson,Jonathan J. Fortney,Neil Miller,Brice-Olivier Demory,Debra A. Fischer,Elisabeth R. Adams,Andrea K. Dupree,Steve B. Howell,Rea Kolbl,John Asher Johnson,Elliott P. Horch,Mark E. Everett,Daniel C. Fabrycky,Sara Seager +17 more
TL;DR: In this article, the authors measured the mass of a modestly irradiated giant planet, KOI-94d, which is in a 22-day orbit and receives 2700 times as much incident flux as Jupiter, and determined that it is not inflated.