G
Gábor Fűrész
Researcher at Massachusetts Institute of Technology
Publications - 50
Citations - 3225
Gábor Fűrész is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Stars & Radial velocity. The author has an hindex of 27, co-authored 50 publications receiving 2858 citations. Previous affiliations of Gábor Fűrész include University of Szeged & Harvard University.
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HAT-P-16b: A 4 MJ PLANET TRANSITING A BRIGHT STAR ON AN ECCENTRIC ORBIT
Lars A. Buchhave,Lars A. Buchhave,Gáspár Á. Bakos,Joel D. Hartman,Guillermo Torres,Gábor L. Kovács,D. W. Latham,Robert W. Noyes,Gil Esquerdo,Mark E. Everett,Andrew W. Howard,G. W. Marcy,Debra A. Fischer,John Asher Johnson,Johannes Andersen,Gábor Fűrész,G. Perumpilly,Dimitar Sasselov,Robert P. Stefanik,B. Béky,J. Lázár,I. Papp,P. Sári +22 more
TL;DR: In this article, the authors reported the discovery of a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch T_c = 2455027.
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KELT-1b: A STRONGLY IRRADIATED, HIGHLY INFLATED, SHORT PERIOD, 27 JUPITER-MASS COMPANION TRANSITING A MID-F STAR
Robert J. Siverd,Thomas G. Beatty,Joshua Pepper,Jason D. Eastman,Jason D. Eastman,Karen A. Collins,Allyson Bieryla,David W. Latham,Lars A. Buchhave,Lars A. Buchhave,Eric L. N. Jensen,Justin R. Crepp,Justin R. Crepp,Rachel Street,Keivan G. Stassun,Keivan G. Stassun,B. Scott Gaudi,Perry Berlind,Michael L. Calkins,Darren L. DePoy,Gilbert A. Esquerdo,Benjamin J. Fulton,Benjamin J. Fulton,Gábor Fűrész,John C. Geary,Andrew Gould,Leslie Hebb,John F. Kielkopf,Jennifer L. Marshall,Richard W. Pogge,K. Z. Stanek,Robert P. Stefanik,Andrew Szentgyorgyi,Mark Trueblood,Patricia Trueblood,Amelia M. Stutz,Amelia M. Stutz,Jennifer L. van Saders +37 more
TL;DR: The first transiting low-mass companion from the wide-field Kilodegree Extremely Little Telescope-North (KELT-North) transit survey was discovered in this paper.
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State of the Field: Extreme Precision Radial Velocities*
Debra A. Fischer,Guillem Anglada-Escudé,Guillem Anglada-Escudé,Pamela Arriagada,Roman V. Baluev,Jacob L. Bean,François Bouchy,Lars A. Buchhave,T. A. Carroll,Abhijit Chakraborty,Justin R. Crepp,Rebekah I. Dawson,Scott A. Diddams,Scott A. Diddams,Xavier Dumusque,Jason D. Eastman,Michael Endl,Pedro Figueira,Eric B. Ford,Daniel Foreman-Mackey,Daniel Foreman-Mackey,Paul Fournier,Gábor Fűrész,B. Scott Gaudi,P. C. Gregory,Frank Grundahl,Artie P. Hatzes,Guillaume Hébrard,Guillaume Hébrard,Enrique Herrero,David W. Hogg,Andrew W. Howard,John Asher Johnson,Paul Jorden,C. Jurgenson,David W. Latham,Greg Laughlin,Thomas J. Loredo,Christophe Lovis,Suvrath Mahadevan,T. M. McCracken,Francesco Pepe,Mario R. Perez,David F. Phillips,Peter Plavchan,Lisa Prato,Andreas Quirrenbach,Ansgar Reiners,Paul Robertson,Nuno C. Santos,David Sawyer,Damien Ségransan,Alessandro Sozzetti,Tilo Steinmetz,Andrew Szentgyorgyi,Stéphane Udry,Jeff A. Valenti,Sharon X. Wang,Robert A. Wittenmyer,Robert A. Wittenmyer,Jason T. Wright +60 more
TL;DR: The Second Workshop on Extreme Precision Radial Velocities defined circa 2015 the state of the art Doppler precision and identified the critical path challenges for reaching 10 cm s−1 measurement precision as mentioned in this paper.
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Kinematic structure of the orion nebula cluster and its surroundings
Gábor Fűrész,Gábor Fűrész,Lee Hartmann,S. Thomas Megeath,Andrew Szentgyorgyi,Erika T. Hamden +5 more
TL;DR: In this paper, high-resolution spectra of 1215 stars in the Orion Nebula Cluster (ONC) and the surrounding Orion 1c association, obtained with the Hectochelle multiobject echelle spectrograph on the 6.5 m MMT, were used to confirm 1111 stars as members, based on their radial velocity and/or Hα emission.
Journal ArticleDOI
TWO “b”s IN THE BEEHIVE: THE DISCOVERY OF THE FIRST HOT JUPITERS IN AN OPEN CLUSTER
Samuel N. Quinn,Russel White,David W. Latham,Lars A. Buchhave,Justin R. Cantrell,S. E. Dahm,Gábor Fűrész,Andrew Szentgyorgyi,John C. Geary,Guillermo Torres,Allyson Bieryla,Perry Berlind,M. C. Calkins,Gilbert A. Esquerdo,Robert P. Stefanik +14 more
TL;DR: The first known hot Jupiters in an open cluster and the only planets known to orbit Sun-like, main-sequence stars in a cluster were detected from Doppler-shifted radial velocities as mentioned in this paper.