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Distance determination for RAVE stars using stellar models

Identifieur interne : 007938 ( Main/Exploration ); précédent : 007937; suivant : 007939

Distance determination for RAVE stars using stellar models

Auteurs : M. A. Breddels [Pays-Bas] ; M. C. Smith [Pays-Bas, République populaire de Chine, Royaume-Uni] ; A. Helmi [Pays-Bas] ; O. Bienayme [France] ; J. Binney [Royaume-Uni] ; J. Bland-Hawthorn [Australie] ; C. Boeche [Allemagne] ; B. C. M. Burnett [Royaume-Uni] ; R. Campbell [Allemagne] ; K. C. Freeman [Australie] ; B. Gibson [Royaume-Uni] ; G. Gilmore [Royaume-Uni] ; E. K. Grebel [Allemagne] ; U. Munari [Italie] ; J. F. Navarro [Canada] ; Q. A. Parker [Australie] ; G. M. Seabroke [Royaume-Uni] ; A. Siebert [France] ; A. Siviero [Allemagne, Italie] ; M. Steinmetz [Allemagne] ; F. G. Watson [Australie] ; M. Williams [Allemagne] ; R. F. G. Wyse [États-Unis] ; T. Zwitter [Slovénie]

Source :

RBID : Pascal:10-0258264

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English descriptors

Abstract

Aims. We develop a method for deriving distances from spectroscopic data and obtaining full 6D phase-space coordinates for the RAVE survey's second data release. Methods. We used stellar models combined with atmospheric properties from RAVE (effective temperature, surface gravity and metallicity) and (J - Ks) photometry from archival sources to derive absolute magnitudes. In combination with apparent magnitudes, sky coordinates, proper motions from a variety of sources and radial velocities from RAVE, we are able to derive the full 6D phase-space coordinates for a large sample of RAVE stars. This method is tested with artificial data, Hipparcos trigonometric parallaxes and observations of the open cluster M 67. Results. When we applied our method to a set of 16 146 stars, we found that 25% (4037) of the stars have relative (statistical) distance errors of <35%, while 50% (8073) and 75% (12 110) have relative (statistical) errors smaller than 45% and 50%, respectively. Our various tests show that we can reliably estimate distances for main-sequence stars, but there is an indication of potential systematic problems with giant stars owing to uncertainties in the underlying stellar models. For the main-sequence star sample (defined as those with log(g) > 4), 25% (1744) have relative distance errors <31%, while 50% (3488) and 75% (5231) have relative errors smaller than 36% and 42%, respectively. Our full dataset shows the expected decrease in the metallicity of stars as a function of distance from the Galactic plane. The known kinematic substructures in the U and V velocity components of nearby dwarf stars are apparent in our dataset, confirming the accuracy of our data and the reliability of our technique. We provide independent measurements of the orientation of the UV velocity ellipsoid and of the solar motion, and they are in very good agreement with previous work. Conclusions. The distance catalogue for the RAVE second data release is available at http: //www. astro. rug. nl/∼rave, and will be updated in the future to include new data releases.


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<orgName type="university">Université de Groningue</orgName>
<placeName>
<settlement type="city">Groningue (ville)</settlement>
<region>Groningue (province)</region>
</placeName>
</affiliation>
<affiliation wicri:level="4">
<inist:fA14 i1="02">
<s1>Kavli Institute for Astronomy and Astrophysics, Peking University</s1>
<s2>Beijing 100871</s2>
<s3>CHN</s3>
<sZ>2 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
<settlement type="city">Pékin</settlement>
</placeName>
<orgName type="university">Université de Pékin</orgName>
</affiliation>
<affiliation wicri:level="4">
<inist:fA14 i1="03">
<s1>Institute of Astronomy, University of Cambridge</s1>
<s2>Cambridge</s2>
<s3>GBR</s3>
<sZ>2 aut.</sZ>
<sZ>12 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<placeName>
<settlement type="city">Cambridge</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Angleterre de l'Est</region>
</placeName>
<orgName type="university">Université de Cambridge</orgName>
</affiliation>
</author>
<author>
<name sortKey="Helmi, A" sort="Helmi, A" uniqKey="Helmi A" first="A." last="Helmi">A. Helmi</name>
<affiliation wicri:level="4">
<inist:fA14 i1="01">
<s1>Kapteyn Astronomical Institute, University of Groningen, PO Box 800</s1>
<s2>9700 AV Groningen</s2>
<s3>NLD</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
<country>Pays-Bas</country>
<wicri:noRegion>9700 AV Groningen</wicri:noRegion>
<orgName type="university">Université de Groningue</orgName>
<placeName>
<settlement type="city">Groningue (ville)</settlement>
<region>Groningue (province)</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Bienayme, O" sort="Bienayme, O" uniqKey="Bienayme O" first="O." last="Bienayme">O. Bienayme</name>
<affiliation wicri:level="4">
<inist:fA14 i1="04">
<s1>Université de Strasbourg, Observatoire Astronomique</s1>
<s2>Strasbourg</s2>
<s3>FRA</s3>
<sZ>4 aut.</sZ>
<sZ>18 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName>
<region type="region">Grand Est</region>
<region type="old region">Alsace (région administrative)</region>
<settlement type="city">Strasbourg</settlement>
<settlement type="city">Strasbourg</settlement>
</placeName>
<orgName type="university">Université de Strasbourg</orgName>
</affiliation>
</author>
<author>
<name sortKey="Binney, J" sort="Binney, J" uniqKey="Binney J" first="J." last="Binney">J. Binney</name>
<affiliation wicri:level="3">
<inist:fA14 i1="05">
<s1>Rudolf Peierls Centre for Theoretical Physics</s1>
<s2>Oxford</s2>
<s3>GBR</s3>
<sZ>5 aut.</sZ>
<sZ>8 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<placeName>
<settlement type="city">Oxford</settlement>
<region type="country">Angleterre</region>
<region type="comté" nuts="2">Oxfordshire</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Bland Hawthorn, J" sort="Bland Hawthorn, J" uniqKey="Bland Hawthorn J" first="J." last="Bland-Hawthorn">J. Bland-Hawthorn</name>
<affiliation wicri:level="3">
<inist:fA14 i1="06">
<s1>Anglo-Australian Observatory</s1>
<s2>Sydney</s2>
<s3>AUS</s3>
<sZ>6 aut.</sZ>
<sZ>21 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<placeName>
<settlement type="city">Sydney</settlement>
<region type="état">Nouvelle-Galles du Sud</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Boeche, C" sort="Boeche, C" uniqKey="Boeche C" first="C." last="Boeche">C. Boeche</name>
<affiliation wicri:level="3">
<inist:fA14 i1="07">
<s1>Astrophysikalisches Institut Potsdam</s1>
<s2>Potsdam</s2>
<s3>DEU</s3>
<sZ>7 aut.</sZ>
<sZ>9 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="2">Brandebourg</region>
<settlement type="city">Potsdam</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Burnett, B C M" sort="Burnett, B C M" uniqKey="Burnett B" first="B. C. M." last="Burnett">B. C. M. Burnett</name>
<affiliation wicri:level="3">
<inist:fA14 i1="05">
<s1>Rudolf Peierls Centre for Theoretical Physics</s1>
<s2>Oxford</s2>
<s3>GBR</s3>
<sZ>5 aut.</sZ>
<sZ>8 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<placeName>
<settlement type="city">Oxford</settlement>
<region type="country">Angleterre</region>
<region type="comté" nuts="2">Oxfordshire</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Campbell, R" sort="Campbell, R" uniqKey="Campbell R" first="R." last="Campbell">R. Campbell</name>
<affiliation wicri:level="3">
<inist:fA14 i1="07">
<s1>Astrophysikalisches Institut Potsdam</s1>
<s2>Potsdam</s2>
<s3>DEU</s3>
<sZ>7 aut.</sZ>
<sZ>9 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="2">Brandebourg</region>
<settlement type="city">Potsdam</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Freeman, K C" sort="Freeman, K C" uniqKey="Freeman K" first="K. C." last="Freeman">K. C. Freeman</name>
<affiliation wicri:level="1">
<inist:fA14 i1="08">
<s1>RSAA, Australian National University</s1>
<s2>Canberra</s2>
<s3>AUS</s3>
<sZ>10 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<wicri:noRegion>Canberra</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Gibson, B" sort="Gibson, B" uniqKey="Gibson B" first="B." last="Gibson">B. Gibson</name>
<affiliation wicri:level="1">
<inist:fA14 i1="09">
<s1>University of Central Lancashire</s1>
<s2>Preston</s2>
<s3>GBR</s3>
<sZ>11 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>University of Central Lancashire</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Gilmore, G" sort="Gilmore, G" uniqKey="Gilmore G" first="G." last="Gilmore">G. Gilmore</name>
<affiliation wicri:level="4">
<inist:fA14 i1="03">
<s1>Institute of Astronomy, University of Cambridge</s1>
<s2>Cambridge</s2>
<s3>GBR</s3>
<sZ>2 aut.</sZ>
<sZ>12 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<placeName>
<settlement type="city">Cambridge</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Angleterre de l'Est</region>
</placeName>
<orgName type="university">Université de Cambridge</orgName>
</affiliation>
</author>
<author>
<name sortKey="Grebel, E K" sort="Grebel, E K" uniqKey="Grebel E" first="E. K." last="Grebel">E. K. Grebel</name>
<affiliation wicri:level="3">
<inist:fA14 i1="10">
<s1>Astronomisches Rechen-Institut, Center for Astronomy of the University of Heidelberg</s1>
<s2>Heidelberg</s2>
<s3>DEU</s3>
<sZ>13 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="1">Bade-Wurtemberg</region>
<region type="district" nuts="2">District de Karlsruhe</region>
<settlement type="city">Heidelberg</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Munari, U" sort="Munari, U" uniqKey="Munari U" first="U." last="Munari">U. Munari</name>
<affiliation wicri:level="1">
<inist:fA14 i1="11">
<s1>INAF, Astronomical Observatory of Padova</s1>
<s2>Asiago station</s2>
<s3>ITA</s3>
<sZ>14 aut.</sZ>
<sZ>19 aut.</sZ>
</inist:fA14>
<country>Italie</country>
<wicri:noRegion>Asiago station</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Navarro, J F" sort="Navarro, J F" uniqKey="Navarro J" first="J. F." last="Navarro">J. F. Navarro</name>
<affiliation wicri:level="1">
<inist:fA14 i1="12">
<s1>University of Victoria</s1>
<s2>Victoria</s2>
<s3>CAN</s3>
<sZ>15 aut.</sZ>
</inist:fA14>
<country>Canada</country>
<wicri:noRegion>University of Victoria</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Parker, Q A" sort="Parker, Q A" uniqKey="Parker Q" first="Q. A." last="Parker">Q. A. Parker</name>
<affiliation wicri:level="3">
<inist:fA14 i1="13">
<s1>Macquarie University</s1>
<s2>Sydney</s2>
<s3>AUS</s3>
<sZ>16 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<placeName>
<settlement type="city">Sydney</settlement>
<region type="état">Nouvelle-Galles du Sud</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Seabroke, G M" sort="Seabroke, G M" uniqKey="Seabroke G" first="G. M." last="Seabroke">G. M. Seabroke</name>
<affiliation wicri:level="1">
<inist:fA14 i1="14">
<s1>ECentre for Electronic Imaging, Planetary and Space Sciences Research Institute, The Open University</s1>
<s2>Milton Keynes</s2>
<s3>GBR</s3>
<sZ>17 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Milton Keynes</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Siebert, A" sort="Siebert, A" uniqKey="Siebert A" first="A." last="Siebert">A. Siebert</name>
<affiliation wicri:level="4">
<inist:fA14 i1="04">
<s1>Université de Strasbourg, Observatoire Astronomique</s1>
<s2>Strasbourg</s2>
<s3>FRA</s3>
<sZ>4 aut.</sZ>
<sZ>18 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName>
<region type="region">Grand Est</region>
<region type="old region">Alsace (région administrative)</region>
<settlement type="city">Strasbourg</settlement>
<settlement type="city">Strasbourg</settlement>
</placeName>
<orgName type="university">Université de Strasbourg</orgName>
</affiliation>
</author>
<author>
<name sortKey="Siviero, A" sort="Siviero, A" uniqKey="Siviero A" first="A." last="Siviero">A. Siviero</name>
<affiliation wicri:level="3">
<inist:fA14 i1="07">
<s1>Astrophysikalisches Institut Potsdam</s1>
<s2>Potsdam</s2>
<s3>DEU</s3>
<sZ>7 aut.</sZ>
<sZ>9 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="2">Brandebourg</region>
<settlement type="city">Potsdam</settlement>
</placeName>
</affiliation>
<affiliation wicri:level="1">
<inist:fA14 i1="11">
<s1>INAF, Astronomical Observatory of Padova</s1>
<s2>Asiago station</s2>
<s3>ITA</s3>
<sZ>14 aut.</sZ>
<sZ>19 aut.</sZ>
</inist:fA14>
<country>Italie</country>
<wicri:noRegion>Asiago station</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Steinmetz, M" sort="Steinmetz, M" uniqKey="Steinmetz M" first="M." last="Steinmetz">M. Steinmetz</name>
<affiliation wicri:level="3">
<inist:fA14 i1="07">
<s1>Astrophysikalisches Institut Potsdam</s1>
<s2>Potsdam</s2>
<s3>DEU</s3>
<sZ>7 aut.</sZ>
<sZ>9 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="2">Brandebourg</region>
<settlement type="city">Potsdam</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Watson, F G" sort="Watson, F G" uniqKey="Watson F" first="F. G." last="Watson">F. G. Watson</name>
<affiliation wicri:level="3">
<inist:fA14 i1="06">
<s1>Anglo-Australian Observatory</s1>
<s2>Sydney</s2>
<s3>AUS</s3>
<sZ>6 aut.</sZ>
<sZ>21 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<placeName>
<settlement type="city">Sydney</settlement>
<region type="état">Nouvelle-Galles du Sud</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Williams, M" sort="Williams, M" uniqKey="Williams M" first="M." last="Williams">M. Williams</name>
<affiliation wicri:level="3">
<inist:fA14 i1="07">
<s1>Astrophysikalisches Institut Potsdam</s1>
<s2>Potsdam</s2>
<s3>DEU</s3>
<sZ>7 aut.</sZ>
<sZ>9 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName>
<region type="land" nuts="2">Brandebourg</region>
<settlement type="city">Potsdam</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Wyse, R F G" sort="Wyse, R F G" uniqKey="Wyse R" first="R. F. G." last="Wyse">R. F. G. Wyse</name>
<affiliation wicri:level="1">
<inist:fA14 i1="15">
<s1>Johns Hopkins University</s1>
<s2>Baltimore, MD</s2>
<s3>USA</s3>
<sZ>23 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Johns Hopkins University</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Zwitter, T" sort="Zwitter, T" uniqKey="Zwitter T" first="T." last="Zwitter">T. Zwitter</name>
<affiliation wicri:level="1">
<inist:fA14 i1="16">
<s1>Faculty of Mathematics and Physics, University of Ljubljana</s1>
<s2>Ljubljana</s2>
<s3>SVN</s3>
<sZ>24 aut.</sZ>
</inist:fA14>
<country>Slovénie</country>
<wicri:noRegion>Ljubljana</wicri:noRegion>
</affiliation>
</author>
</analytic>
<series>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
<imprint>
<date when="2010">2010</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Absolute magnitude</term>
<term>Astronomical catalogues</term>
<term>Distance measurement</term>
<term>Dwarf stars</term>
<term>Dynamics</term>
<term>Effective temperature</term>
<term>Ellipsoid</term>
<term>Galactic planes</term>
<term>Galaxies</term>
<term>Galaxy structure</term>
<term>Giant stars</term>
<term>Kinematics</term>
<term>Main sequence stars</term>
<term>Metallicity</term>
<term>Nearby stars</term>
<term>Numerical method</term>
<term>Open clusters</term>
<term>Phase space</term>
<term>Photometry</term>
<term>Proper motion</term>
<term>Radial velocity</term>
<term>Star clusters</term>
<term>Star models</term>
<term>Statistical method</term>
<term>Substructure</term>
<term>Surface gravity</term>
<term>Uncertainty</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Mesure distance</term>
<term>Modèle stellaire</term>
<term>Espace phase</term>
<term>Température effective</term>
<term>Gravité surface</term>
<term>Métallicité</term>
<term>Photométrie</term>
<term>Magnitude absolue</term>
<term>Mouvement propre</term>
<term>Vitesse radiale</term>
<term>Amas ouvert</term>
<term>Etoile séquence principale</term>
<term>Etoile géante</term>
<term>Incertitude</term>
<term>Plan galactique</term>
<term>Cinématique</term>
<term>Sous structure</term>
<term>Etoile proche</term>
<term>Etoile naine</term>
<term>Ellipsoïde</term>
<term>Catalogue astronomique</term>
<term>Méthode numérique</term>
<term>Méthode statistique</term>
<term>Galaxies</term>
<term>Dynamique</term>
<term>Structure galaxies</term>
<term>Amas stellaire</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Méthode statistique</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">Aims. We develop a method for deriving distances from spectroscopic data and obtaining full 6D phase-space coordinates for the RAVE survey's second data release. Methods. We used stellar models combined with atmospheric properties from RAVE (effective temperature, surface gravity and metallicity) and (J - K
<sub>s</sub>
) photometry from archival sources to derive absolute magnitudes. In combination with apparent magnitudes, sky coordinates, proper motions from a variety of sources and radial velocities from RAVE, we are able to derive the full 6D phase-space coordinates for a large sample of RAVE stars. This method is tested with artificial data, Hipparcos trigonometric parallaxes and observations of the open cluster M 67. Results. When we applied our method to a set of 16 146 stars, we found that 25% (4037) of the stars have relative (statistical) distance errors of <35%, while 50% (8073) and 75% (12 110) have relative (statistical) errors smaller than 45% and 50%, respectively. Our various tests show that we can reliably estimate distances for main-sequence stars, but there is an indication of potential systematic problems with giant stars owing to uncertainties in the underlying stellar models. For the main-sequence star sample (defined as those with log(g) > 4), 25% (1744) have relative distance errors <31%, while 50% (3488) and 75% (5231) have relative errors smaller than 36% and 42%, respectively. Our full dataset shows the expected decrease in the metallicity of stars as a function of distance from the Galactic plane. The known kinematic substructures in the U and V velocity components of nearby dwarf stars are apparent in our dataset, confirming the accuracy of our data and the reliability of our technique. We provide independent measurements of the orientation of the UV velocity ellipsoid and of the solar motion, and they are in very good agreement with previous work. Conclusions. The distance catalogue for the RAVE second data release is available at http: //www. astro. rug. nl/∼rave, and will be updated in the future to include new data releases.</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>Allemagne</li>
<li>Australie</li>
<li>Canada</li>
<li>France</li>
<li>Italie</li>
<li>Pays-Bas</li>
<li>Royaume-Uni</li>
<li>République populaire de Chine</li>
<li>Slovénie</li>
<li>États-Unis</li>
</country>
<region>
<li>Alsace (région administrative)</li>
<li>Angleterre</li>
<li>Angleterre de l'Est</li>
<li>Bade-Wurtemberg</li>
<li>Brandebourg</li>
<li>District de Karlsruhe</li>
<li>Grand Est</li>
<li>Groningue (province)</li>
<li>Nouvelle-Galles du Sud</li>
<li>Oxfordshire</li>
</region>
<settlement>
<li>Cambridge</li>
<li>Groningue (ville)</li>
<li>Heidelberg</li>
<li>Oxford</li>
<li>Potsdam</li>
<li>Pékin</li>
<li>Strasbourg</li>
<li>Sydney</li>
</settlement>
<orgName>
<li>Université de Cambridge</li>
<li>Université de Groningue</li>
<li>Université de Pékin</li>
<li>Université de Strasbourg</li>
</orgName>
</list>
<tree>
<country name="Pays-Bas">
<region name="Groningue (province)">
<name sortKey="Breddels, M A" sort="Breddels, M A" uniqKey="Breddels M" first="M. A." last="Breddels">M. A. Breddels</name>
</region>
<name sortKey="Helmi, A" sort="Helmi, A" uniqKey="Helmi A" first="A." last="Helmi">A. Helmi</name>
<name sortKey="Smith, M C" sort="Smith, M C" uniqKey="Smith M" first="M. C." last="Smith">M. C. Smith</name>
</country>
<country name="République populaire de Chine">
<noRegion>
<name sortKey="Smith, M C" sort="Smith, M C" uniqKey="Smith M" first="M. C." last="Smith">M. C. Smith</name>
</noRegion>
</country>
<country name="Royaume-Uni">
<region name="Angleterre">
<name sortKey="Smith, M C" sort="Smith, M C" uniqKey="Smith M" first="M. C." last="Smith">M. C. Smith</name>
</region>
<name sortKey="Binney, J" sort="Binney, J" uniqKey="Binney J" first="J." last="Binney">J. Binney</name>
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<name sortKey="Gibson, B" sort="Gibson, B" uniqKey="Gibson B" first="B." last="Gibson">B. Gibson</name>
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