R
Ronald L. Gilliland
Researcher at Pennsylvania State University
Publications - 223
Citations - 43218
Ronald L. Gilliland is an academic researcher from Pennsylvania State University. The author has contributed to research in topics: Planet & Stars. The author has an hindex of 94, co-authored 223 publications receiving 41200 citations. Previous affiliations of Ronald L. Gilliland include Space Telescope Science Institute.
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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
Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data
Natalie M. Batalha,Natalie M. Batalha,Jason F. Rowe,Stephen T. Bryson,Thomas Barclay,Christopher J. Burke,Douglas A. Caldwell,Jessie L. Christiansen,Fergal Mullally,Susan E. Thompson,Timothy M. Brown,Andrea K. Dupree,Daniel C. Fabrycky,Eric B. Ford,Jonathan J. Fortney,Ronald L. Gilliland,Howard Isaacson,David W. Latham,Geoffrey W. Marcy,Samuel N. Quinn,Samuel N. Quinn,Darin Ragozzine,Avi Shporer,William J. Borucki,David R. Ciardi,Thomas N. Gautier,Michael R. Haas,Jon M. Jenkins,David G. Koch,Jack J. Lissauer,William Rapin,Gibor Basri,Alan P. Boss,Lars A. Buchhave,Joshua A. Carter,David Charbonneau,Joergen Christensen-Dalsgaard,Bruce D. Clarke,William D. Cochran,Brice-Olivier Demory,Jean-Michel Desert,Edna DeVore,Laurance R. Doyle,Gilbert A. Esquerdo,Mark E. Everett,Francois Fressin,John C. Geary,Forrest R. Girouard,Alan Gould,Jennifer R. Hall,Matthew J. Holman,Andrew W. Howard,Steve B. Howell,Khadeejah A. Ibrahim,Karen Kinemuchi,Hans Kjeldsen,Todd C. Klaus,Jie Li,Philip W. Lucas,Søren Meibom,Robert L. Morris,Andrej Prsa,Elisa V. Quintana,Dwight T. Sanderfer,Dimitar Sasselov,Shawn Seader,Jeffrey C. Smith,Jason H. Steffen,Martin Still,Martin C. Stumpe,Jill Tarter,Peter Tenenbaum,Guillermo Torres,Joseph D. Twicken,Kamal Uddin,Jeffrey Van Cleve,Lucianne M. Walkowicz,William F. Welsh +77 more
TL;DR: In this paper, the authors verified nearly 5000 periodic transit-like signals against astrophysical and instrumental false positives yielding 1108 viable new transiting planet candidates, bringing the total count up to over 2300.
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
The photometric performance and calibration of the Hubble Space Telescope advanced camera for surveys
Marco Sirianni,Marco Sirianni,Marco Sirianni,Myungkook J. Jee,Narciso Benítez,Narciso Benítez,John P. Blakeslee,André R. Martel,Gerhardt R. Meurer,M. Clampin,G. De Marchi,G. De Marchi,G. De Marchi,Holland C. Ford,Ronald L. Gilliland,George F. Hartig,Garth D. Illingworth,J. Mack,Wm. J. McCann +18 more
TL;DR: In this paper, the photometric calibration of the Advanced Camera for Surveys (ACS) was presented, and a significant amount of data has been collected to characterize the on-orbit performance of the three channels.
Journal ArticleDOI
Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data
Natalie M. Batalha,Jason F. Rowe,Stephen T. Bryson,Thomas Barclay,Christopher J. Burke,Douglas A. Caldwell,Jessie L. Christiansen,Fergal Mullally,Susan E. Thompson,Timothy M. Brown,Andrea K. Dupree,Daniel C. Fabrycky,Eric B. Ford,Jonathan J. Fortney,Ronald L. Gilliland,Howard Isaacson,David W. Latham,Geoffrey W. Marcy,Samuel N. Quinn,Samuel N. Quinn,Darin Ragozzine,Avi Shporer,William J. Borucki,David R. Ciardi,Thomas N. Gautier,Michael R. Haas,Jon M. Jenkins,David G. Koch,Jack J. Lissauer,William Rapin,Gibor Basri,Alan P. Boss,Lars A. Buchhave,David Charbonneau,Joergen Christensen-Dalsgaard,Bruce D. Clarke,William D. Cochran,Brice-Olivier Demory,Edna DeVore,Gilbert A. Esquerdo,Mark E. Everett,Francois Fressin,John C. Geary,Forrest R. Girouard,Alan Gould,Jennifer R. Hall,Matthew J. Holman,Andrew W. Howard,Steve B. Howell,Khadeejah A. Ibrahim,Karen Kinemuchi,Hans Kjeldsen,Todd C. Klaus,Jie Li,Philip W. Lucas,Robert L. Morris,Andrej Prsa,Elisa V. Quintana,Dwight T. Sanderfer,Dimitar Sasselov,Shawn Seader,Jeffrey C. Smith,Jason H. Steffen,Martin Still,Martin C. Stumpe,Jill Tarter,Peter Tenenbaum,Guillermo Torres,Joseph D. Twicken,Kamal Uddin,Jeffrey Van Cleve,Lucianne M. Walkowicz,William F. Welsh +72 more
TL;DR: In this paper, the authors used the noise-weighted robust averaging of multi-quarter photo-center offsets derived from difference image analysis, which identifies likely background eclipsing binaries.