A
Andrew Szentgyorgyi
Researcher at Harvard University
Publications - 151
Citations - 13655
Andrew Szentgyorgyi is an academic researcher from Harvard University. The author has contributed to research in topics: Spectrograph & Exoplanet. The author has an hindex of 48, co-authored 144 publications receiving 12068 citations.
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Journal ArticleDOI
Transiting Exoplanet Survey Satellite
George R. Ricker,Joshua N. Winn,Roland Vanderspek,David W. Latham,Gáspár Á. Bakos,Jacob L. Bean,Zachory K. Berta-Thompson,Timothy M. Brown,Lars A. Buchhave,Lars A. Buchhave,Nathaniel R. Butler,R. Paul Butler,William J. Chaplin,William J. Chaplin,David Charbonneau,Jørgen Christensen-Dalsgaard,Mark Clampin,Drake Deming,John P. Doty,Nathan De Lee,Nathan De Lee,Courtney D. Dressing,Edward W. Dunham,Michael Endl,Francois Fressin,Jian Ge,Thomas Henning,Matthew J. Holman,Andrew W. Howard,Shigeru Ida,Jon M. Jenkins,G. Jernigan,John Asher Johnson,Lisa Kaltenegger,Nobuyuki Kawai,Hans Kjeldsen,Gregory Laughlin,Alan M. Levine,Douglas N. C. Lin,Jack J. Lissauer,Phillip J. MacQueen,Geoffrey W. Marcy,Peter R. McCullough,Peter R. McCullough,Timothy D. Morton,Norio Narita,Martin Paegert,Enric Palle,Francesco Pepe,Joshua Pepper,Joshua Pepper,Andreas Quirrenbach,Stephen A. Rinehart,Dimitar Sasselov,Bun'ei Sato,Sara Seager,Alessandro Sozzetti,Keivan G. Stassun,Keivan G. Stassun,Peter Sullivan,Andrew Szentgyorgyi,Guillermo Torres,Stéphane Udry,Joel Villasenor +63 more
TL;DR: The Transiting Exoplanet Survey Satellite (TESS) as discussed by the authors will search for planets transiting bright and nearby stars using four wide-field optical charge-coupled device cameras to monitor at least 200,000 main-sequence dwarf stars.
Journal ArticleDOI
The Transiting Exoplanet Survey Satellite
George R. Ricker,Joshua N. Winn,Roland Vanderspek,David W. Latham,Gáspár Á. Bakos,Jacob L. Bean,Zachory K. Berta-Thompson,Timothy M. Brown,Lars A. Buchhave,Nathaniel R. Butler,R. Paul Butler,William J. Chaplin,David Charbonneau,Jørgen Christensen-Dalsgaard,Mark Clampin,Drake Deming,John P. Doty,Nathan De Lee,Courtney D. Dressing,Edward W. Dunham,Michael Endl,Francois Fressin,Jian Ge,Thomas Henning,Matthew J. Holman,Andrew W. Howard,Shigeru Ida,Jon M. Jenkins,G. Jernigan,John Asher Johnson,Lisa Kaltenegger,Nobuyuki Kawai,Hans Kjeldsen,Gregory Laughlin,Alan M. Levine,Douglas N. C. Lin,Jack J. Lissauer,Phillip J. MacQueen,Geoffrey W. Marcy,Peter R. McCullough,Timothy D. Morton,Norio Narita,Martin Paegert,Enric Palle,Francesco Pepe,Joshua Pepper,Andreas Quirrenbach,S. A. Rinehart,Dimitar Sasselov,Bun'ei Sato,Sara Seager,Alessandro Sozzetti,Keivan G. Stassun,Peter Sullivan,Andrew Szentgyorgyi,Guillermo Torres,Stéphane Udry,Joel Villasenor +57 more
TL;DR: The Transiting Exoplanet Survey Satellite (TESS) as mentioned in this paper was selected by NASA for launch in 2017 as an Astrophysics Explorer mission to search for planets transiting bright and nearby stars.
Proceedings ArticleDOI
Transiting Exoplanet Survey Satellite (TESS)
George R. Ricker,Joshua N. Winn,Roland Vanderspek,David W. Latham,Gáspár Á. Bakos,Jacob L. Bean,Zachory K. Berta-Thompson,Timothy M. Brown,Lars A. Buchhave,Lars A. Buchhave,Nathaniel R. Butler,R. Paul Butler,William J. Chaplin,William J. Chaplin,David Charbonneau,Jørgen Christensen-Dalsgaard,Mark Clampin,Drake Deming,John P. Doty,Nathan De Lee,Nathan De Lee,Courtney D. Dressing,Edward W. Dunham,Michael Endl,Francois Fressin,Jian Ge,Thomas Henning,Matthew J. Holman,Andrew W. Howard,Shigeru Ida,Jon M. Jenkins,G. Jernigan,John Asher Johnson,Lisa Kaltenegger,Nobuyuki Kawai,Hans Kjeldsen,Gregory Laughlin,Alan M. Levine,Douglas N. C. Lin,Jack J. Lissauer,Phillip J. MacQueen,Geoffrey W. Marcy,Peter R. McCullough,Peter R. McCullough,Timothy D. Morton,Norio Narita,Martin Paegert,Enric Palle,Francesco Pepe,Joshua Pepper,Joshua Pepper,Andreas Quirrenbach,Stephen A. Rinehart,Dimitar Sasselov,Bun'ei Sato,Sara Seager,Alessandro Sozzetti,Keivan G. Stassun,Keivan G. Stassun,Peter Sullivan,Andrew Szentgyorgyi,Guillermo Torres,Stéphane Udry,Joel Villasenor +63 more
TL;DR: The Transiting Exoplanet Survey Satellite (TESS) as mentioned in this paper will discover thousands of exoplanets in orbit around the brightest stars in the sky, including Earth-sized to gas giants, around a wide range of stellar types and orbital distances.
Journal ArticleDOI
CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA
Malcolm Hicken,Peter Challis,Saurabh Jha,Robert P. Kirshner,Thomas Matheson,Maryam Modjaz,A. Rest,W. Michael Wood-Vasey,Gáspár Á. Bakos,Elizabeth J. Barton,Perry Berlind,Ann Bragg,Cesar Briceno,Warren R. Brown,Nelson Caldwell,Mike Calkins,Richard Cho,Larry Ciupik,M. E. Contreras,Kristi Dendy,A. Dosaj,Nick Durham,Kris Eriksen,G. A. Esquerdo,Mark E. Everett,Emilio E. Falco,J. M. Fernandez,Alejandro E. Gaba,Peter M. Garnavich,Genevieve J. Graves,Paul J. Green,Ted Groner,Carl Hergenrother,Matthew J. Holman,Vit Hradecky,John P. Huchra,Bob Hutchison,D. Jerius,Andrés Jordán,Roy Kilgard,Miriam I. Krauss,Kevin Luhman,Lucas M. Macri,Daniel P. Marrone,Jonathan C. McDowell,Daniel H. McIntosh,Brian R. McNamara,Tom Megeath,B. J. Mochejska,Diego J. Muñoz,James Muzerolle,Orlando Naranjo,Gautham Narayan,Michael A. Pahre,Wayne Peters,D. E. Peterson,Kenneth J. Rines,Ben Ripman,Anna Roussanova,Rudolph E. Schild,Aurora Sicilia-Aguilar,J. L. Sokoloski,Kyle Smalley,A. W. Smith,Tim Spahr,Krzysztof Z. Stanek,Pauline Barmby,Stephane Blondin,Christopher W. Stubbs,Andrew Szentgyorgyi,Manuel A. P. Torres,Amili Vaz,Alexey Vikhlinin,Zhong Wang,Mike Westover,Deborah Freedman Woods,Ping Zhao +76 more
TL;DR: In this article, the authors present multiband photometry of 185 type-Ia supernovae (SNe Ia), with over 11,500 observations acquired between 2001 and 2008 at the F. L. Whipple Observatory of Harvard-Smithsonian Center for Astrophysics (CfA).
Journal ArticleDOI
A laser frequency comb that enables radial velocity measurements with a precision of 1 cm s -1
Chih-Hao Li,Andrew Benedick,Peter Fendel,Alexander G. Glenday,Franz X. Kärtner,David F. Phillips,Dimitar Sasselov,Andrew Szentgyorgyi,Ronald L. Walsworth +8 more
TL;DR: The fabrication of a filtered laser comb with up to 40-GHz (∼1-Å) line spacing, generated from a 1-GHz repetition-rate source, without compromising long-term stability, reproducibility or spectral resolution is reported.