C
Craig Kulesa
Researcher at University of Arizona
Publications - 177
Citations - 7859
Craig Kulesa is an academic researcher from University of Arizona. The author has contributed to research in topics: Telescope & Star formation. The author has an hindex of 42, co-authored 171 publications receiving 7574 citations. Previous affiliations of Craig Kulesa include Steward Health Care System & Max Planck Society.
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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
FIRST LIGHT LBT AO IMAGES OF HR 8799 bcde AT 1.6 AND 3.3 μm: NEW DISCREPANCIES BETWEEN YOUNG PLANETS AND OLD BROWN DWARFS*
Andrew J. Skemer,Philip M. Hinz,Simone Esposito,Adam Burrows,Jarron Leisenring,Michael F. Skrutskie,Silvano Desidera,Dino Mesa,Carmelo Arcidiacono,Filippo Mannucci,Timothy J. Rodigas,Laird M. Close,Donald W. McCarthy,Craig Kulesa,Guido Agapito,Daniel Apai,Javier Argomedo,Vanessa P. Bailey,K. Boutsia,Runa Briguglio,Guido Brusa,Lorenzo Busoni,Riccardo Claudi,Joshua Eisner,Luca Fini,Katherine B. Follette,Peter M. Garnavich,Raffaele Gratton,J. C. Guerra,John M. Hill,William F. Hoffmann,Terry J. Jones,M. Krejny,Jared R. Males,Elena Masciadri,Michael Meyer,Douglas L. Miller,Katie M. Morzinski,Matthew J. Nelson,Enrico Pinna,Alfio Puglisi,Sascha P. Quanz,Fernando Quiros-Pacheco,Armando Riccardi,P. Stefanini,Vidhya Vaitheeswaran,John C. Wilson,Marco Xompero +47 more
TL;DR: In this paper, the spectral energy distribution of the HR 8799 planets is modeled as a mixture of clouds of varying opacity, similar to the patchy cloud structures on Jupiter and L/T transition brown dwarfs.
Journal ArticleDOI
First Light LBT AO Images of HR 8799 bcde at 1.65 and 3.3 Microns: New Discrepancies between Young Planets and Old Brown Dwarfs
Andrew J. Skemer,Philip M. Hinz,Simone Esposito,Adam Burrows,Jarron Leisenring,Michael F. Skrutskie,Silvano Desidera,Dino Mesa,Carmelo Arcidiacono,Filippo Mannucci,Timothy J. Rodigas,Laird M. Close,Donald W. McCarthy,Craig Kulesa,Guido Agapito,Daniel Apai,Javier Argomedo,Vanessa P. Bailey,K. Boutsia,Runa Briguglio,Guido Brusa,Lorenzo Busoni,Riccardo Claudi,Joshua Eisner,Luca Fini,Katherine B. Follette,Peter M. Garnavich,Raffaele Gratton,Juan Carlos Guerra,John M. Hill,William F. Hoffmann,Terry Jones,Megan Krejny,Jared R. Males,Elena Masciadri,Michael Meyer,Douglas L. Miller,Katie M. Morzinski,Matthew J. Nelson,Enrico Pinna,Alfio Puglisi,Sascha P. Quanz,Fernando Quiros-Pacheco,Armando Riccardi,P. Stefanini,Vidhya Vaitheeswaran,John C. Wilson,Marco Xompero +47 more
TL;DR: In this paper, the authors used the LBT adaptive optics system, PISCES, and LBTI/LMIRCam to image all four of the HR 8799 planets at H-band and 3.3 microns.
Journal ArticleDOI
An Imaging Survey for Extrasolar Planets around 45 Close, Young Stars with the Simultaneous Differential Imager at the Very Large Telescope and MMT
Beth Biller,Laird M. Close,Elena Masciadri,Eric L. Nielsen,Rainer Lenzen,Wolfgang Brandner,Donald W. McCarthy,Markus Hartung,Markus Hartung,S. Kellner,Eric E. Mamajek,Thomas Henning,Douglas L. Miller,Matthew A. Kenworthy,Craig Kulesa +14 more
TL;DR: In this article, the authors present the results of a survey of 45 young (P250Myr), close (P50pc) stars with the Simultaneous Differential Imager (SDI) implemented at the VLT and the MMT for direct detection of extrasolar planets.