D
Donald W. McCarthy
Researcher at University of Arizona
Publications - 213
Citations - 9627
Donald W. McCarthy is an academic researcher from University of Arizona. The author has contributed to research in topics: Telescope & Adaptive optics. The author has an hindex of 47, co-authored 208 publications receiving 9340 citations. Previous affiliations of Donald W. McCarthy include Steward Health Care System & Association of Universities for Research in Astronomy.
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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
A Standard Stellar Spectral Sequence in the Red/Near-Infrared: Classes K5 to M9
TL;DR: In this paper, the spectral slopes and the strengths of the red/near-infrared spectral features are used to distinguish giants from dwarfs and to classify M dwarfs of all spectral subclasses.
Journal ArticleDOI
The mass-luminosity relation for stars of mass 1.0 to 0.08 solar mass
TL;DR: In this paper, the mass-visual luminosity relation for stars with 2.0-0.08 solar mass is obtained by implementing new photometric relations linking V to JHK wavelengths, supplemented with eclipsing binary information.
Journal ArticleDOI
The Multiplicity of Pre-Main-Sequence Stars in Southern Star-forming Regions
Andrea M. Ghez,Donald W. McCarthy,Donald W. McCarthy,Jennifer Patience,Tracy L. Beck,Tracy L. Beck +5 more
TL;DR: In this article, a K-band multiplicity survey of pre-main-sequence stars located in the dark cloud complexes Chameleon, Lupus, and Corona Australis was carried out with both speckle and direct-imaging techniques.