The RAdial Velocity Experiment (RAVE): Fourth data release

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 atmo...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2013-09
Hauptverfasser: Kordopatis, G, Gilmore, G, Steinmetz, M, Boeche, C, Seabroke, G M, Siebert, A, Zwitter, T, Binney, J, de Laverny, P, Recio-Blanco, A, Williams, M E K, Piffl, T, Enke, H, Roeser, S, Bijaoui, A, Wyse, R F G, Freeman, K, Munari, U, Carillo, I, Anguiano, B, Burton, D, Campbell, R, Cass, C J P, Fiegert, K, Hartley, M, Parker, Q A, Reid, W, Ritter, A, Russell, K S, Stupart, M, Watson, F G, Bienayme, O, Bland-Hawthorn, J, Gerhard, O, Gibson, B K, Grebel, E K, Helmi, A, Navarro, J F, Conrad, C, Famaey, B, Faure, C, Just, A, Kos, J, Matijevic, G, McMillan, P J, Minchev, I, Scholz, R, Sharma, S, Siviero, A, Wylie de Boer, E, Zerjal, M
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Kordopatis, G
Gilmore, G
Steinmetz, M
Boeche, C
Seabroke, G M
Siebert, A
Zwitter, T
Binney, J
de Laverny, P
Recio-Blanco, A
Williams, M E K
Piffl, T
Enke, H
Roeser, S
Bijaoui, A
Wyse, R F G
Freeman, K
Munari, U
Carillo, I
Anguiano, B
Burton, D
Campbell, R
Cass, C J P
Fiegert, K
Hartley, M
Parker, Q A
Reid, W
Ritter, A
Russell, K S
Stupart, M
Watson, F G
Bienayme, O
Bland-Hawthorn, J
Gerhard, O
Gibson, B K
Grebel, E K
Helmi, A
Navarro, J F
Conrad, C
Famaey, B
Faure, C
Just, A
Kos, J
Matijevic, G
McMillan, P J
Minchev, I
Scholz, R
Sharma, S
Siviero, A
Wylie de Boer, E
Zerjal, M
description 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 2MASS 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 which 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 website and the Vizier database.
doi_str_mv 10.48550/arxiv.1309.4284
format Article
fullrecord <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1309_4284</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2082694689</sourcerecordid><originalsourceid>FETCH-LOGICAL-a519-e85cecd511eb9e09f5f536bfafcd6aa2bc527f41aa4b1ccb1972274626cbd0093</originalsourceid><addsrcrecordid>eNotj01Lw0AURQdBsNTuXcmAG10kzrz5SKa7UlIVCkIJ3YaXyQtNiU1MUmn_val1dTeHyzmMPUgR6tgY8YrdqfoJpRIu1BDrGzYBpWQQa4A7Nuv7vRACbATGqAmbpzvim0VRYc23VDe-Gs48ObXUVV90GPjzZrFNXuZ81Ry7YccLHJB3VBP2dM9uS6x7mv3vlKWrJF2-B-vPt4_lYh2gkS6g2HjyhZGSckfClaY0yuYllr6wiJB7A1GpJaLOpfe5dBFApC1YnxdCODVlj9fbv66sHcWwO2eXvuzSNwJPV6Dtmu8j9UO2H2UPo1IGIgbrtI2d-gVdTFGo</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2082694689</pqid></control><display><type>article</type><title>The RAdial Velocity Experiment (RAVE): Fourth data release</title><source>arXiv.org</source><source>Free E- Journals</source><creator>Kordopatis, G ; Gilmore, G ; Steinmetz, M ; Boeche, C ; Seabroke, G M ; Siebert, A ; Zwitter, T ; Binney, J ; de Laverny, P ; Recio-Blanco, A ; Williams, M E K ; Piffl, T ; Enke, H ; Roeser, S ; Bijaoui, A ; Wyse, R F G ; Freeman, K ; Munari, U ; Carillo, I ; Anguiano, B ; Burton, D ; Campbell, R ; Cass, C J P ; Fiegert, K ; Hartley, M ; Parker, Q A ; Reid, W ; Ritter, A ; Russell, K S ; Stupart, M ; Watson, F G ; Bienayme, O ; Bland-Hawthorn, J ; Gerhard, O ; Gibson, B K ; Grebel, E K ; Helmi, A ; Navarro, J F ; Conrad, C ; Famaey, B ; Faure, C ; Just, A ; Kos, J ; Matijevic, G ; McMillan, P J ; Minchev, I ; Scholz, R ; Sharma, S ; Siviero, A ; Wylie de Boer, E ; Zerjal, M</creator><creatorcontrib>Kordopatis, G ; Gilmore, G ; Steinmetz, M ; Boeche, C ; Seabroke, G M ; Siebert, A ; Zwitter, T ; Binney, J ; de Laverny, P ; Recio-Blanco, A ; Williams, M E K ; Piffl, T ; Enke, H ; Roeser, S ; Bijaoui, A ; Wyse, R F G ; Freeman, K ; Munari, U ; Carillo, I ; Anguiano, B ; Burton, D ; Campbell, R ; Cass, C J P ; Fiegert, K ; Hartley, M ; Parker, Q A ; Reid, W ; Ritter, A ; Russell, K S ; Stupart, M ; Watson, F G ; Bienayme, O ; Bland-Hawthorn, J ; Gerhard, O ; Gibson, B K ; Grebel, E K ; Helmi, A ; Navarro, J F ; Conrad, C ; Famaey, B ; Faure, C ; Just, A ; Kos, J ; Matijevic, G ; McMillan, P J ; Minchev, I ; Scholz, R ; Sharma, S ; Siviero, A ; Wylie de Boer, E ; Zerjal, M</creatorcontrib><description>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 2MASS 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 which 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 website and the Vizier database.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1309.4284</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Algorithms ; Aluminum ; Magnesium ; Metallicity ; Organic chemistry ; Parameters ; Photometry ; Physics - Astrophysics of Galaxies ; Physics - Solar and Stellar Astrophysics ; Radial velocity ; Titanium ; Websites</subject><ispartof>arXiv.org, 2013-09</ispartof><rights>2013. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27924</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1309.4284$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1088/0004-6256/146/5/134$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Kordopatis, G</creatorcontrib><creatorcontrib>Gilmore, G</creatorcontrib><creatorcontrib>Steinmetz, M</creatorcontrib><creatorcontrib>Boeche, C</creatorcontrib><creatorcontrib>Seabroke, G M</creatorcontrib><creatorcontrib>Siebert, A</creatorcontrib><creatorcontrib>Zwitter, T</creatorcontrib><creatorcontrib>Binney, J</creatorcontrib><creatorcontrib>de Laverny, P</creatorcontrib><creatorcontrib>Recio-Blanco, A</creatorcontrib><creatorcontrib>Williams, M E K</creatorcontrib><creatorcontrib>Piffl, T</creatorcontrib><creatorcontrib>Enke, H</creatorcontrib><creatorcontrib>Roeser, S</creatorcontrib><creatorcontrib>Bijaoui, A</creatorcontrib><creatorcontrib>Wyse, R F G</creatorcontrib><creatorcontrib>Freeman, K</creatorcontrib><creatorcontrib>Munari, U</creatorcontrib><creatorcontrib>Carillo, I</creatorcontrib><creatorcontrib>Anguiano, B</creatorcontrib><creatorcontrib>Burton, D</creatorcontrib><creatorcontrib>Campbell, R</creatorcontrib><creatorcontrib>Cass, C J P</creatorcontrib><creatorcontrib>Fiegert, K</creatorcontrib><creatorcontrib>Hartley, M</creatorcontrib><creatorcontrib>Parker, Q A</creatorcontrib><creatorcontrib>Reid, W</creatorcontrib><creatorcontrib>Ritter, A</creatorcontrib><creatorcontrib>Russell, K S</creatorcontrib><creatorcontrib>Stupart, M</creatorcontrib><creatorcontrib>Watson, F G</creatorcontrib><creatorcontrib>Bienayme, O</creatorcontrib><creatorcontrib>Bland-Hawthorn, J</creatorcontrib><creatorcontrib>Gerhard, O</creatorcontrib><creatorcontrib>Gibson, B K</creatorcontrib><creatorcontrib>Grebel, E K</creatorcontrib><creatorcontrib>Helmi, A</creatorcontrib><creatorcontrib>Navarro, J F</creatorcontrib><creatorcontrib>Conrad, C</creatorcontrib><creatorcontrib>Famaey, B</creatorcontrib><creatorcontrib>Faure, C</creatorcontrib><creatorcontrib>Just, A</creatorcontrib><creatorcontrib>Kos, J</creatorcontrib><creatorcontrib>Matijevic, G</creatorcontrib><creatorcontrib>McMillan, P J</creatorcontrib><creatorcontrib>Minchev, I</creatorcontrib><creatorcontrib>Scholz, R</creatorcontrib><creatorcontrib>Sharma, S</creatorcontrib><creatorcontrib>Siviero, A</creatorcontrib><creatorcontrib>Wylie de Boer, E</creatorcontrib><creatorcontrib>Zerjal, M</creatorcontrib><title>The RAdial Velocity Experiment (RAVE): Fourth data release</title><title>arXiv.org</title><description>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 2MASS 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 which 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 website and the Vizier database.</description><subject>Algorithms</subject><subject>Aluminum</subject><subject>Magnesium</subject><subject>Metallicity</subject><subject>Organic chemistry</subject><subject>Parameters</subject><subject>Photometry</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Radial velocity</subject><subject>Titanium</subject><subject>Websites</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotj01Lw0AURQdBsNTuXcmAG10kzrz5SKa7UlIVCkIJ3YaXyQtNiU1MUmn_val1dTeHyzmMPUgR6tgY8YrdqfoJpRIu1BDrGzYBpWQQa4A7Nuv7vRACbATGqAmbpzvim0VRYc23VDe-Gs48ObXUVV90GPjzZrFNXuZ81Ry7YccLHJB3VBP2dM9uS6x7mv3vlKWrJF2-B-vPt4_lYh2gkS6g2HjyhZGSckfClaY0yuYllr6wiJB7A1GpJaLOpfe5dBFApC1YnxdCODVlj9fbv66sHcWwO2eXvuzSNwJPV6Dtmu8j9UO2H2UPo1IGIgbrtI2d-gVdTFGo</recordid><startdate>20130917</startdate><enddate>20130917</enddate><creator>Kordopatis, G</creator><creator>Gilmore, G</creator><creator>Steinmetz, M</creator><creator>Boeche, C</creator><creator>Seabroke, G M</creator><creator>Siebert, A</creator><creator>Zwitter, T</creator><creator>Binney, J</creator><creator>de Laverny, P</creator><creator>Recio-Blanco, A</creator><creator>Williams, M E K</creator><creator>Piffl, T</creator><creator>Enke, H</creator><creator>Roeser, S</creator><creator>Bijaoui, A</creator><creator>Wyse, R F G</creator><creator>Freeman, K</creator><creator>Munari, U</creator><creator>Carillo, I</creator><creator>Anguiano, B</creator><creator>Burton, D</creator><creator>Campbell, R</creator><creator>Cass, C J P</creator><creator>Fiegert, K</creator><creator>Hartley, M</creator><creator>Parker, Q A</creator><creator>Reid, W</creator><creator>Ritter, A</creator><creator>Russell, K S</creator><creator>Stupart, M</creator><creator>Watson, F G</creator><creator>Bienayme, O</creator><creator>Bland-Hawthorn, J</creator><creator>Gerhard, O</creator><creator>Gibson, B K</creator><creator>Grebel, E K</creator><creator>Helmi, A</creator><creator>Navarro, J F</creator><creator>Conrad, C</creator><creator>Famaey, B</creator><creator>Faure, C</creator><creator>Just, A</creator><creator>Kos, J</creator><creator>Matijevic, G</creator><creator>McMillan, P J</creator><creator>Minchev, I</creator><creator>Scholz, R</creator><creator>Sharma, S</creator><creator>Siviero, A</creator><creator>Wylie de Boer, E</creator><creator>Zerjal, M</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20130917</creationdate><title>The RAdial Velocity Experiment (RAVE): Fourth data release</title><author>Kordopatis, G ; Gilmore, G ; Steinmetz, M ; Boeche, C ; Seabroke, G M ; Siebert, A ; Zwitter, T ; Binney, J ; de Laverny, P ; Recio-Blanco, A ; Williams, M E K ; Piffl, T ; Enke, H ; Roeser, S ; Bijaoui, A ; Wyse, R F G ; Freeman, K ; Munari, U ; Carillo, I ; Anguiano, B ; Burton, D ; Campbell, R ; Cass, C J P ; Fiegert, K ; Hartley, M ; Parker, Q A ; Reid, W ; Ritter, A ; Russell, K S ; Stupart, M ; Watson, F G ; Bienayme, O ; Bland-Hawthorn, J ; Gerhard, O ; Gibson, B K ; Grebel, E K ; Helmi, A ; Navarro, J F ; Conrad, C ; Famaey, B ; Faure, C ; Just, A ; Kos, J ; Matijevic, G ; McMillan, P J ; Minchev, I ; Scholz, R ; Sharma, S ; Siviero, A ; Wylie de Boer, E ; Zerjal, M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a519-e85cecd511eb9e09f5f536bfafcd6aa2bc527f41aa4b1ccb1972274626cbd0093</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Algorithms</topic><topic>Aluminum</topic><topic>Magnesium</topic><topic>Metallicity</topic><topic>Organic chemistry</topic><topic>Parameters</topic><topic>Photometry</topic><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Solar and Stellar Astrophysics</topic><topic>Radial velocity</topic><topic>Titanium</topic><topic>Websites</topic><toplevel>online_resources</toplevel><creatorcontrib>Kordopatis, G</creatorcontrib><creatorcontrib>Gilmore, G</creatorcontrib><creatorcontrib>Steinmetz, M</creatorcontrib><creatorcontrib>Boeche, C</creatorcontrib><creatorcontrib>Seabroke, G M</creatorcontrib><creatorcontrib>Siebert, A</creatorcontrib><creatorcontrib>Zwitter, T</creatorcontrib><creatorcontrib>Binney, J</creatorcontrib><creatorcontrib>de Laverny, P</creatorcontrib><creatorcontrib>Recio-Blanco, A</creatorcontrib><creatorcontrib>Williams, M E K</creatorcontrib><creatorcontrib>Piffl, T</creatorcontrib><creatorcontrib>Enke, H</creatorcontrib><creatorcontrib>Roeser, S</creatorcontrib><creatorcontrib>Bijaoui, A</creatorcontrib><creatorcontrib>Wyse, R F G</creatorcontrib><creatorcontrib>Freeman, K</creatorcontrib><creatorcontrib>Munari, U</creatorcontrib><creatorcontrib>Carillo, I</creatorcontrib><creatorcontrib>Anguiano, B</creatorcontrib><creatorcontrib>Burton, D</creatorcontrib><creatorcontrib>Campbell, R</creatorcontrib><creatorcontrib>Cass, C J P</creatorcontrib><creatorcontrib>Fiegert, K</creatorcontrib><creatorcontrib>Hartley, M</creatorcontrib><creatorcontrib>Parker, Q A</creatorcontrib><creatorcontrib>Reid, W</creatorcontrib><creatorcontrib>Ritter, A</creatorcontrib><creatorcontrib>Russell, K S</creatorcontrib><creatorcontrib>Stupart, M</creatorcontrib><creatorcontrib>Watson, F G</creatorcontrib><creatorcontrib>Bienayme, O</creatorcontrib><creatorcontrib>Bland-Hawthorn, J</creatorcontrib><creatorcontrib>Gerhard, O</creatorcontrib><creatorcontrib>Gibson, B K</creatorcontrib><creatorcontrib>Grebel, E K</creatorcontrib><creatorcontrib>Helmi, A</creatorcontrib><creatorcontrib>Navarro, J F</creatorcontrib><creatorcontrib>Conrad, C</creatorcontrib><creatorcontrib>Famaey, B</creatorcontrib><creatorcontrib>Faure, C</creatorcontrib><creatorcontrib>Just, A</creatorcontrib><creatorcontrib>Kos, J</creatorcontrib><creatorcontrib>Matijevic, G</creatorcontrib><creatorcontrib>McMillan, P J</creatorcontrib><creatorcontrib>Minchev, I</creatorcontrib><creatorcontrib>Scholz, R</creatorcontrib><creatorcontrib>Sharma, S</creatorcontrib><creatorcontrib>Siviero, A</creatorcontrib><creatorcontrib>Wylie de Boer, E</creatorcontrib><creatorcontrib>Zerjal, M</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kordopatis, G</au><au>Gilmore, G</au><au>Steinmetz, M</au><au>Boeche, C</au><au>Seabroke, G M</au><au>Siebert, A</au><au>Zwitter, T</au><au>Binney, J</au><au>de Laverny, P</au><au>Recio-Blanco, A</au><au>Williams, M E K</au><au>Piffl, T</au><au>Enke, H</au><au>Roeser, S</au><au>Bijaoui, A</au><au>Wyse, R F G</au><au>Freeman, K</au><au>Munari, U</au><au>Carillo, I</au><au>Anguiano, B</au><au>Burton, D</au><au>Campbell, R</au><au>Cass, C J P</au><au>Fiegert, K</au><au>Hartley, M</au><au>Parker, Q A</au><au>Reid, W</au><au>Ritter, A</au><au>Russell, K S</au><au>Stupart, M</au><au>Watson, F G</au><au>Bienayme, O</au><au>Bland-Hawthorn, J</au><au>Gerhard, O</au><au>Gibson, B K</au><au>Grebel, E K</au><au>Helmi, A</au><au>Navarro, J F</au><au>Conrad, C</au><au>Famaey, B</au><au>Faure, C</au><au>Just, A</au><au>Kos, J</au><au>Matijevic, G</au><au>McMillan, P J</au><au>Minchev, I</au><au>Scholz, R</au><au>Sharma, S</au><au>Siviero, A</au><au>Wylie de Boer, E</au><au>Zerjal, M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The RAdial Velocity Experiment (RAVE): Fourth data release</atitle><jtitle>arXiv.org</jtitle><date>2013-09-17</date><risdate>2013</risdate><eissn>2331-8422</eissn><abstract>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 2MASS 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 which 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 website and the Vizier database.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1309.4284</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2013-09
issn 2331-8422
language eng
recordid cdi_arxiv_primary_1309_4284
source arXiv.org; Free E- Journals
subjects Algorithms
Aluminum
Magnesium
Metallicity
Organic chemistry
Parameters
Photometry
Physics - Astrophysics of Galaxies
Physics - Solar and Stellar Astrophysics
Radial velocity
Titanium
Websites
title The RAdial Velocity Experiment (RAVE): Fourth data release
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-11T08%3A46%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20RAdial%20Velocity%20Experiment%20(RAVE):%20Fourth%20data%20release&rft.jtitle=arXiv.org&rft.au=Kordopatis,%20G&rft.date=2013-09-17&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1309.4284&rft_dat=%3Cproquest_arxiv%3E2082694689%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2082694689&rft_id=info:pmid/&rfr_iscdi=true