J
J. P. Fulbright
Researcher at Johns Hopkins University
Publications - 13
Citations - 2268
J. P. Fulbright is an academic researcher from Johns Hopkins University. The author has contributed to research in topics: Radial velocity & Globular cluster. The author has an hindex of 12, co-authored 13 publications receiving 2079 citations. Previous affiliations of J. P. Fulbright include University of California, Santa Cruz.
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Journal ArticleDOI
The radial velocity experiment (RAVE): First data release
Matthias Steinmetz,A. Siebert,Harry Enke,Corrado Boeche,Andreas Kelz,R.-D. Scholz,Von Berlepsch R,Tomaž Zwitter,U. Jauregi,L. Mijovic,Daniel J. Eisenstein,F. G. Watson,Quentin A. Parker,D. Burton,Cjp Cass,J. A. Dawe,Kristin Fiegert,M. Hartley,K. S. Russell,Will Saunders,Joss Bland-Hawthorn,Kenneth C. Freeman,M. Williams,Ulisse Munari,M. Fiorucci,Alessandro Siviero,Rosanna Sordo,Randy D. Campbell,George M. Seabroke,Gerry Gilmore,Nick Evans,Genevieve Parmentier,S. Vidrih,R. F. G. Wyse,Olivier Bienaymé,L. Veltz,Siegfried Roeser,J. P. Fulbright,G. R. Ruchti,Elena Schilbach,Brad K. Gibson,Eva K. Grebel,Ortwin Gerhard,Amina Helmi,Matthew Smith,Julio F. Navarro,J. Penarrubia,Jeremy Bailin,James Binney,Walter Dehnen,Ivan Minchev,Alice C. Quillen,Mike Read,B. J. Boyle +53 more
TL;DR: The first data release of the Radial Velocity Experiment (RAVE) is presented and it is demonstrated that the radial velocities derived for the first data set do not show any systematic trend with color or signal-to-noise ratio.
Journal ArticleDOI
The Radial Velocity Experiment (RAVE)
Matthias Steinmetz,Tomaz Zwitter,A. Siebert,F. G. Watson,Kenneth C. Freeman,U. Munari,Randy D. Campbell,M. Williams,George M. Seabroke,Rosemary F. G. Wyse,Quentin A. Parker,Olivier Bienaymé,Siegfried Roeser,Brad K. Gibson,Gerry Gilmore,Eva K. Grebel,Julio F. Navarro,D. Burton,C. J. P. Cass,J. A. Dawe,Kristin Fiegert,M. Hartley,K. S. Russell,Will Saunders,Harry Enke,Jeremy Bailin,James Binney,Joss Bland-Hawthorn,Corrado Boeche,W. Dehnen,Daniel J. Eisenstein,Nick Evans,M. Fiorucci,J. P. Fulbright,Ortwin Gerhard,U. Jauregi,A. Kelz,L. Mijovic,Ivan Minchev,Genevieve Parmentier,J. Penarrubia,Alice C. Quillen,Mike Read,Gregory R. Ruchti,Ralf-Dieter Scholz,Alessandro Siviero,M. C. Smith,Rosanna Sordo,L. Veltz,S. Vidrih,R. von Berlepsch,B. J. Boyle,Elena Schilbach,Amina Helmi +53 more
Journal ArticleDOI
The two metallicity groups of the globular cluster M 22: a chemical perspective
Anna F. Marino,Christopher Sneden,Robert P. Kraft,George Wallerstein,John E. Norris,G. S. Da Costa,Antonino Milone,Antonino Milone,Inese I. Ivans,Guillermo Gonzalez,Guillermo Gonzalez,J. P. Fulbright,J. P. Fulbright,Michael Hilker,Giampaolo Piotto,Manuela Zoccali,P. B. Stetson +16 more
TL;DR: In this article, a detailed chemical composition analysis of 35 red giant stars in the globular cluster M22 is presented, in which two stellar groups are characterized by a di erent content in iron, neutron capture elements Y, Zr and Ba, and element Ca.
Journal ArticleDOI
The two metallicity groups of the globular cluster M22: a chemical perspective
A. F. Marino,Christopher Sneden,Robert P. Kraft,George Wallerstein,John E. Norris,G. S. Da Costa,A. P. Milone,Inese I. Ivans,Guillermo A. González,J. P. Fulbright,Michael Hilker,G. Piotto,M. Zoccali,P. B. Stetson +13 more
TL;DR: In this article, a detailed chemical composition analysis of 35 red giant stars in the globular cluster M22 is presented, in which two stellar groups are characterized by a different content in iron, neutron capture elements Y, Zr and Ba, and alpha element Ca.
Journal ArticleDOI
Observational Properties of the Metal-poor Thick Disk of the Milky Way and Insights into its Origins
Gregory R. Ruchti,J. P. Fulbright,Rosemary F. G. Wyse,Gerard Gilmore,Olivier Bienaymé,Joss Bland-Hawthorn,Brad K. Gibson,Eva K. Grebel,Amina Helmi,Ulisse Munari,Julio F. Navarro,Quentin A. Parker,Warren A. Reid,George M. Seabroke,Arnaud Siebert,Alessandro Siviero,Matthias Steinmetz,Fred G. Watson,Mary E K Williams,Tomaž Zwitter +19 more
TL;DR: In this paper, a sample of 214 red giant branch, 31 red clump/horizontal branch, and 74 main-sequence/sub-giant branch metal-poor stars was used to investigate the gradients in the metalpoor thick disk.