G
Gil Esquerdo
Researcher at Harvard University
Publications - 61
Citations - 4243
Gil Esquerdo is an academic researcher from Harvard University. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 33, co-authored 61 publications receiving 3907 citations. Previous affiliations of Gil Esquerdo include Planetary Science Institute.
Papers
More filters
Journal ArticleDOI
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.
Journal ArticleDOI
The Transit Light Curve Project. IX. Evidence for a Smaller Radius of the Exoplanet XO-3b
Joshua N. Winn,Matthew J. Holman,Guillermo Torres,Peter R. McCullough,Christopher M. Johns-Krull,David W. Latham,Avi Shporer,Tsevi Mazeh,Enrique Garcia-Melendo,Cindy N. Foote,Gil Esquerdo,Mark E. Everett +11 more
TL;DR: In this article, the authors present photometry of 13 transits of XO-3b, a massive transiting planet on an eccentric orbit, and revise the system parameters accordingly.
Journal ArticleDOI
HAT-P-1b: A Large-Radius, Low-Density Exoplanet Transiting One Member of a Stellar Binary* **
Gáspár Á. Bakos,Robert W. Noyes,Géza Kovács,David W. Latham,Dimitar Sasselov,Guillermo Torres,Debra A. Fischer,Robert P. Stefanik,Bun'ei Sato,John Asher Johnson,András Pál,András Pál,G. W. Marcy,R. P. Butler,Gil Esquerdo,Krzysztof Z. Stanek,J. Lazar,I. Papp,Pál Sári,B. Sipőcz,B. Sipőcz +20 more
TL;DR: In this article, the authors used small automated telescopes in Arizona and Hawaii to detect an object transiting one member of the double star system ADS 16402, which is a pair of G0 main-sequence stars with age about 3 Gyr at a distance of ~139 pc and projected separation of ~1550 AU.
Journal ArticleDOI
HAT-P-7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field
András Pál,András Pál,Gáspár Á. Bakos,Guillermo Torres,Robert W. Noyes,D. W. Latham,Géza Kovács,G. W. Marcy,Debra A. Fischer,R. P. Butler,Dimitar Sasselov,B. Sipőcz,B. Sipőcz,Gil Esquerdo,Gábor L. Kovács,Robert P. Stefanik,J. Lazar,I. Papp,Pál Sári +18 more
TL;DR: In this article, the authors reported the discovery of a very hot giant planet orbiting a bright star with a small semimajor axis of 0.0377 ± 0.0005 AU.
Journal ArticleDOI
CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE
Malcolm Hicken,Peter Challis,Robert P. Kirshner,Armin Rest,Claire E. Cramer,W. Michael Wood-Vasey,Gáspár Á. Bakos,Gáspár Á. Bakos,Perry Berlind,Warren R. Brown,Nelson Caldwell,Mike Calkins,Thayne Currie,Katherine de Kleer,Gil Esquerdo,Mark E. Everett,Emilio E. Falco,J. M. Fernandez,Andrew S. Friedman,Ted Groner,Joel D. Hartman,Joel D. Hartman,Matthew J. Holman,R. Hutchins,Sonia Keys,David M. Kipping,D. W. Latham,George H Marion,Gautham Narayan,Michael A. Pahre,András Pál,Wayne Peters,G. Perumpilly,Ben Ripman,Brigitta Sipocz,Andrew Szentgyorgyi,S. Tang,Manuel A. P. Torres,A. Vaz,Scott J. Wolk,Andreas Zezas +40 more
TL;DR: In this article, multi-band optical photometry of 94 spectroscopically confirmed Type Ia supernovae (SNe Ia) in the redshift range 0.0055-0.073 was presented.