J
Jeremy Jones
Researcher at Georgia State University
Publications - 31
Citations - 2977
Jeremy Jones is an academic researcher from Georgia State University. The author has contributed to research in topics: Stars & Reverberation mapping. The author has an hindex of 18, co-authored 30 publications receiving 2812 citations.
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Journal ArticleDOI
Stellar Diameters and Temperatures. II. Main-sequence K- and M-stars
Tabetha S. Boyajian,Kaspar von Braun,Gerard T. van Belle,Harold A. McAlister,T. ten Brummelaar,Stephen R. Kane,Philip S. Muirhead,Jeremy Jones,Russel White,Gail H. Schaefer,David R. Ciardi,Todd J. Henry,Mercedes Lopez-Morales,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,D. H. Berger +24 more
TL;DR: In this article, Boyajian et al. presented interferometric angular diameter measurements of 21 low-mass, K- and M-dwarfs made with the CHARA Array.
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
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.
Journal ArticleDOI
Space Telescope and Optical Reverberation Mapping Project. III. Optical Continuum Emission and Broad-Band Time Delays in NGC 5548
Michael Fausnaugh,Kelly D. Denney,Aaron J. Barth,Misty C. Bentz,M. C. Bottorff,Michael T. Carini,Kevin V. Croxall,G. De Rosa,M. R. Goad,Keith Horne,Michael D. Joner,Shai Kaspi,Mi-Ryang Kim,S. A. Klimanov,Christopher S. Kochanek,Douglas C. Leonard,Hagai Netzer,Bradley M. Peterson,K. Schnülle,S. G. Sergeev,Marianne Vestergaard,W. Zheng,Ying Zu,P. Arévalo,C. Bazhaw,G. A. Borman,Todd A. Boroson,W. N. Brandt,A. A. Breeveld,Brendon J. Brewer,Edward M. Cackett,D. M. Crenshaw,E. Dalla Bontà,A. de Lorenzo-Cáceres,M. Dietrich,Rick Edelson,N. V. Efimova,Justin Ely,Phil Evans,Alexei V. Filippenko,K. Flatland,N. Gehrels,S. Geier,J. M. Gelbord,L. Gonzalez,V. Gorjian,C. J. Grier,Dirk Grupe,Patrick B. Hall,S. Hicks,D. Horenstein,T. Hutchison,M. Im,J. J. Jensen,Jeremy Jones,Jelle Kaastra,Brandon C. Kelly,J. A. Kennea,Sang Chul Kim,K. T. Korista,Gerard A. Kriss,J. C. Lee,P. Lira,F. MacInnis,E. R. Manne-Nicholas,Smita Mathur,I. M. McHardy,C. Montouri,R. Musso,S. V. Nazarov,Ray P. Norris,J. A. Nousek,D. N. Okhmat,A. Pancoast,I. E. Papadakis,J. R. Parks,Liuyi Pei,R. W. Pogge,J.-U. Pott,S. E. Rafter,H. W. Rix,D. A. Saylor,J. S. Schimoia,M. H. Siegel,M. Spencer,D. A. Starkey,Hyun-Il Sung,K. G. Teems,Tommaso Treu,C. S. Turner,Phil Uttley,Carolin Villforth,Y. Weiss,Jong-Hak Woo,Haojing Yan,S. Young +95 more
TL;DR: In this paper, the authors present ground-based optical photometric monitoring data for NGC 5548, part of an extended multi-wavelength reverberation mapping campaign, and confirm significant time delays between the continuum bands as a function of wavelength, extending the wavelength coverage from 1158 to the $z$ band.