G
Gail Schaefer
Researcher at Georgia State University
Publications - 198
Citations - 6334
Gail Schaefer is an academic researcher from Georgia State University. The author has contributed to research in topics: Stars & CHARA array. The author has an hindex of 42, co-authored 174 publications receiving 5841 citations. Previous affiliations of Gail Schaefer include Space Telescope Science Institute & Stony Brook University.
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Journal ArticleDOI
Stellar Diameters and Temperatures II. Main Sequence K & M Stars
Tabetha S. Boyajian,Kaspar von Braun,Gerard van Belle,Harold A. McAlister,T. ten Brummelaar,Stephen R. Kane,Phil Muirhead,Jeremy Jones,Russel White,Gail Schaefer,David R. Ciardi,Todd J. Henry,Mercedes Lopez-Morales,Stephen T. Ridgway,Douglas R. Gies,Wei-Chun Jao,Bárbara Rojas-Ayala,J. Robert Parks,Laszlo Sturmann,Judit Sturmann,Nils H. Turner,Chris Farrington,P. J. Goldfinger,David H. Berger +23 more
TL;DR: In this paper, the authors presented interferometric diameter measurements of 21 K- and M- dwarfs made with the CHARA Array and derived empirical relations between the stellar Teff, radius, and luminosity to broadband color indices and metallicity.
Journal ArticleDOI
Stellar diameters and temperatures. iii. main-sequence a, f, g, and k stars: additional high-precision measurements and empirical relations
Tabetha S. Boyajian,Tabetha S. Boyajian,Kaspar von Braun,Kaspar von Braun,Gerard T. van Belle,Chris Farrington,Gail Schaefer,Jeremy Jones,Russel White,Harold A. McAlister,T. ten Brummelaar,Stephen T. Ridgway,Douglas R. Gies,Laszlo Sturmann,Judit Sturmann,Nils H. Turner,P. J. Goldfinger,Norm Vargas +17 more
TL;DR: In this article, the angular diameters of 23 nearby main-sequence stars, ranging from spectral types A7 to K0, were derived using Hipparcos parallaxes and measured bolometric fluxes.
Journal ArticleDOI
Fundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array
Daniel Huber,Michael Ireland,T. R. Bedding,I. M. Brandão,L. Piau,Vicente Maestro,Timothy R. White,H. Bruntt,Luca Casagrande,Joanna Molenda-Żakowicz,V. Silva Aguirre,S. G. Sousa,Thomas Barclay,Christopher J. Burke,William J. Chaplin,J. Christensen-Dalsgaard,M. S. Cunha,J. De Ridder,Chris Farrington,Antonio Frasca,R. A. Garcia,R. L. Gilliland,P. J. Goldfinger,S. Hekker,Steven D. Kawaler,H. Kjeldsen,H. A. McAlister,T. S. Metcalfe,Andrea Miglio,Mário J. P. F. G. Monteiro,Marc H. Pinsonneault,Gail Schaefer,D. Stello,Martin C. Stumpe,J. Sturmann,L. Sturmann,T. ten Brummelaar,Michael Thompson,Neal J. Turner,K. Uytterhoeven +39 more
TL;DR: In this article, a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array was used to measure the angular sizes of five main-sequence stars, one subgiant and four red giant stars for which solar-like oscillations have been detected by either Kepler or CoRoT.
Journal ArticleDOI
Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA Array
Daniel Huber,Daniel Huber,Michael J. Ireland,Michael J. Ireland,Michael J. Ireland,Timothy R. Bedding,I. M. Brandão,L. Piau,Vicente Maestro,Timothy R. White,H. Bruntt,Luca Casagrande,Joanna Molenda-Żakowicz,V. Silva Aguirre,S. G. Sousa,Thomas Barclay,Christopher J. Burke,William J. Chaplin,William J. Chaplin,Jørgen Christensen-Dalsgaard,Margarida S. Cunha,J. De Ridder,Chris Farrington,Antonio Frasca,Rafael A. García,R. L. Gilliland,P. J. Goldfinger,Saskia Hekker,S. D. Kawaler,Hans Kjeldsen,Harold A. McAlister,Travis S. Metcalfe,Andrea Miglio,Mário J. P. F. G. Monteiro,Marc H. Pinsonneault,Gail Schaefer,Dennis Stello,Martin C. Stumpe,Judit Sturmann,Laszlo Sturmann,T. ten Brummelaar,Michael Thompson,Nils H. Turner,K. Uytterhoeven,K. Uytterhoeven +44 more
TL;DR: In this article, a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array was used to measure the angular sizes of five main-sequence stars, one subgiant and four red giant stars for which solar-like oscillations have been detected by either Kepler or CoRoT.
Journal ArticleDOI
Stellar Diameters and Temperatures III. Main Sequence A, F, G, & K Stars: Additional high-precision measurements and empirical relations
Tabetha S. Boyajian,Kaspar von Braun,Gerard van Belle,Chris Farrington,Gail Schaefer,Jeremy Jones,Russel White,Harold A. McAlister,T. ten Brummelaar,Stephen T. Ridgway,Douglas R. Gies,Laszlo Sturmann,Judit Sturmann,Nils H. Turner,P. J. Goldfinger,Norm Vargas +15 more
TL;DR: In this article, the angular diameters of 23 nearby main-sequence stars, ranging from spectral type A7 to K0, were derived using HIPPARCOS parallaxes and measured bolometric fluxes.