THE RADIAL VELOCITY EXPERIMENT (RAVE): FOURTH DATA RELEASE

被引：296

作者：

Kordopatis, G. ^{[1
]}

Gilmore, G. ^{[1
]}

Steinmetz, M. ^{[2
]}

Boeche, C. ^{[3
]}

Seabroke, G. M. ^{[4
]}

Siebert, A. ^{[5
]}

Zwitter, T. ^{[6
,7
]}

Binney, J. ^{[8
]}

de Laverny, P. ^{[9
]}

Recio-Blanco, A. ^{[9
]}

Williams, M. E. K. ^{[2
]}

Piffl, T. ^{[2
]}

Enke, H. ^{[2
]}

Roeser, S. ^{[3
]}

Bijaoui, A. ^{[9
]}

Wyse, R. F. G. ^{[10
]}

Freeman, K. ^{[11
]}

Munari, U. ^{[12
]}

Carrillo, I. ^{[2
]}

Anguiano, B. ^{[13
,14
]}

Burton, D. ^{[11
,15
]}

Campbell, R. ^{[16
]}

Cass, C. J. P. ^{[15
]}

Fiegert, K. ^{[15
]}

Hartley, M. ^{[15
]}

Parker, Q. A. ^{[13
,14
,17
]}

Reid, W. ^{[14
,17
]}

Ritter, A. ^{[18
]}

Russell, K. S. ^{[15
]}

Stupar, M. ^{[15
]}

Watson, F. G. ^{[15
]}

Bienayme, O. ^{[5
]}

Bland-Hawthorn, J. ^{[19
]}

Gerhard, O. ^{[20
]}

Gibson, B. K. ^{[21
]}

Grebel, E. K. ^{[3
]}

Helmi, A. ^{[22
]}

Navarro, J. F. ^{[23
]}

Conrad, C. ^{[2
]}

Famaey, B. ^{[5
]}

Faure, C. ^{[5
]}

Just, A. ^{[3
]}

Kos, J. ^{[6
]}

Matijevic, G. ^{[6
]}

McMillan, P. J. ^{[8
]}

Minchev, I. ^{[2
]}

Scholz, R. ^{[2
]}

Sharma, S. ^{[19
]}

Siviero, A. ^{[2
]}

de Boer, E. Wylie ^{[11
]}

机构：

[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England

[2] Leibniz Inst Astrophys Potsdam, D-14482 Potsdam, Germany

[3] Heidelberg Univ, Zentrum Astron, Astron Rechen Inst, D-69120 Heidelberg, Germany

[4] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England

[5] Univ Strasbourg, CNRS, Observ Astron Strasbourg, UMR 7550, F-67000 Strasbourg, France

[6] Univ Ljubljana, Fac Math & Phys, Ljubljana 1000, Slovenia

[7] Ctr Excellence SPACE SI, Ljubljana 1000, Slovenia

[8] Rudolf Peierls Ctr Theoret Phys, Oxford OX1 3NP, England

[9] Univ Nice Sophia Antipolis, Lab Lagrange, UMR 7293, Observ Cote Azur,CNRS, F-06304 Nice, France

[10] Johns Hopkins Univ, Baltimore, MD 21218 USA

[11] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia

[12] INAF Natl Inst Astrophys, Astron Inst Padova, I-36012 Asiago, VI, Italy

[13] Australian Astron Observ, N Ryde, NSW 1670, Australia

[14] Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia

[15] Anglo Australian Observ, Epping, NSW 1710, Australia

[16] Western Kentucky Univ, Bowling Green, KY 42101 USA

[17] Macquarie Res Ctr Astron Astrophys & Astrophoton, N Ryde, NSW 2109, Australia

[18] Natl Cent Univ, Zhongli City 325, Taoyuan County, Taiwan

[19] Univ Sydney, Sch Phys A28, Sydney Inst Astron, Sydney, NSW 2006, Australia

[20] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[21] Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England

[22] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands

[23] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada

来源：

ASTRONOMICAL JOURNAL | 2013年 / 146卷 / 05期

基金：

澳大利亚研究理事会; 欧洲研究理事会; 美国国家科学基金会; 加拿大自然科学与工程研究理事会; 瑞士国家科学基金会;

关键词：

catalogs; stars: abundances; stars: fundamental parameters; surveys; techniques: spectroscopic; METAL-POOR STARS; COLLABORATION MONITORING PROGRAM; GENEVA-COPENHAGEN SURVEY; RED GIANT BRANCH; 1ST DATA RELEASE; T-EFF SCALE; SOLAR NEIGHBORHOOD; MILKY-WAY; GALACTIC DISK; NEARBY STARS;

D O I：

10.1088/0004-6256/146/5/134

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, individual abundances, and distances determined for 425,561 stars, which constitute the fourth public data release of the RAdial Velocity Experiment (RAVE). The stellar atmospheric parameters are computed using a new pipeline, based on the algorithms of MATISSE and DEGAS. The spectral degeneracies and the Two Micron All Sky Survey photometric information are now better taken into consideration, improving the parameter determination compared to the previous RAVE data releases. The individual abundances for six elements (magnesium, aluminum, silicon, titanium, iron, and nickel) are also given, based on a special-purpose pipeline that is also improved compared to that available for the RAVE DR3 and Chemical DR1 data releases. Together with photometric information and proper motions, these data can be retrieved from the RAVE collaboration Web site and the Vizier database.

引用

页数：36

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