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Mikkel Nørup Lund

THE RADIAL VELOCITY EXPERIMENT (RAVE): FIFTH DATA RELEASE

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Dokumenter

DOI

  • Andrea Kunder, Leibniz Inst Astrophys Potsdam AIP
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  • Georges Kordopatis, Leibniz Inst Astrophys Potsdam AIP
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  • Matthias Steinmetz, Leibniz Inst Astrophys Potsdam AIP
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  • Tomaz Zwitter, University of Ljubljana
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  • Paul J. McMillan, Lund University
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  • Luca Casagrande, RSSS, Australian National University
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  • Harry Enke, Leibniz Inst Astrophys Potsdam AIP
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  • Jennifer Wojno, Leibniz Inst Astrophys Potsdam AIP
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  • Marica Valentini, Leibniz Inst Astrophys Potsdam AIP
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  • Cristina Chiappini, Leibniz Inst Astrophys Potsdam AIP
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  • Gal MatijeviC, Leibniz Inst Astrophys Potsdam AIP
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  • Alessandro Siviero, Univ Padua, University of Padua, Dept Biol
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  • Patrick de laverny, CNRS Centre National de la Recherche Scientifique
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  • Alejandra Recio-Blanco, CNRS Centre National de la Recherche Scientifique
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  • Albert Bijaoui, CNRS Centre National de la Recherche Scientifique
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  • Rosemary F. G. Wyse, Johns Hopkins University, Baltimore
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  • James Binney, University of Oxford, Oxford
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  • E. K. Grebel, Heidelberg Univ, Ruprecht Karl University Heidelberg, Dept Polit Sci
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  • Amina Helmi, University of Groningen
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  • Paula Jofre, Univ Diego Portales, University Diego Portales, Fac Ingn, Nucleo Astron
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  • Teresa Antoja, University of Groningen
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  • Gerard Gilmore, Univ Diego Portales, University Diego Portales, Fac Ingn, Nucleo Astron
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  • Arnaud Siebert, Univ Strasbourg, University of Strasbourg
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  • Benoit Famaey, Univ Strasbourg, University of Strasbourg
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  • Olivier Bienayme, Univ Strasbourg, University of Strasbourg
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  • Brad K. Gibson, University of Hull
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  • Kenneth C. Freeman, RSSS, Australian National University
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  • Julio F. Navarro, University of Victoria
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  • Ulisse Munari, Univ Padua, University of Padua, Dept Biol
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  • George Seabroke, University College London, London
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  • Borja Anguiano, Macquarie University
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  • Marusa Zerjal, University of Ljubljana
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  • Ivan Minchev, Leibniz Inst Astrophys Potsdam AIP
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  • Warren Reid, University of Western Sydney
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  • Joss Bland-Hawthorn, Sydney University, Sydney
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  • Janez Kos, Sydney University, Sydney
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  • Sanjib Sharma, Sydney University, Sydney
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  • Fred Watson, Anglo Australian Observ
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  • Quentin A. Parker, Chinese University Hong Kong
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  • Ralf-Dieter Scholz, Leibniz Inst Astrophys Potsdam AIP
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  • Donna Burton, Australian Natl Univ, Australian National University, Mt Stromlo Observ, Res Sch Astron & Astrophys
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  • Paul Cass, Australian Natl Univ, Australian National University, Mt Stromlo Observ, Res Sch Astron & Astrophys
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  • Malcolm Hartley, Australian Natl Univ, Australian National University, Mt Stromlo Observ, Res Sch Astron & Astrophys
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  • Kristin Fiegert, Australian Natl Univ, Australian National University, Mt Stromlo Observ, Res Sch Astron & Astrophys
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  • Milorad Stupar, Macquarie University
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  • Andreas Ritter, Princeton University, Princeton, NJ
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  • Keith Hawkins, Columbia University
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  • Ortwin Gerhard, Max Planck Inst Astron, Max Planck Society
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  • W. J. Chaplin, Aarhus Universitet
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  • G. R. Davies, Aarhus Universitet
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  • Y. P. Elsworth, Aarhus Universitet
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  • M. N. Lund
  • A. Miglio
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  • B. Mosser, GEPI, Observatoire de Paris

Data Release 5 (DR5) of the Radial Velocity Experiment (RAVE) is the fifth data release from a magnitude-limited (9 <I <12) survey of stars randomly selected in the Southern Hemisphere. The RAVE medium-resolution spectra (R similar to 7500) covering the Ca-triplet region (8410-8795 ) span the complete time frame from the start of RAVE observations in 2003 to their completion in 2013. Radial velocities from 520,781 spectra of 457,588 unique stars are presented, of which 255,922 stellar observations have parallaxes and proper motions from the Tycho-Gaia astrometric solution in Gaia DR1. For our main DR5 catalog, stellar parameters (effective temperature, surface gravity, and overall metallicity) are computed using the RAVE DR4 stellar pipeline, but calibrated using recent K2 Campaign 1 seismic gravities and Gaia benchmark stars, as well as results obtained from high-resolution studies. Also included are temperatures from the Infrared Flux Method, and we provide a catalog of red giant stars in the dereddened color(J - Ks)(0) interval (0.50, 0.85) for which the gravities were calibrated based only on seismology. Further data products for subsamples of the RAVE stars include individual abundances for Mg, Al, Si, Ca, Ti, Fe, and Ni, and distances found using isochrones. Each RAVE spectrum is complemented by an error spectrum, which has been used to determine uncertainties on the parameters. The data can be accessed via the RAVE Web site or the VizieR database.

OriginalsprogEngelsk
Artikelnummer75
TidsskriftAstronomical Journal
Vol/bind153
Nummer2
Antal sider30
ISSN0004-6256
DOI
StatusUdgivet - feb. 2017

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