Weak Gravitational Lensing
Identifieur interne : 000739 ( Main/Corpus ); précédent : 000738; suivant : 000740Weak Gravitational Lensing
Auteurs : A. HeavensSource :
- Lecture Notes in Physics [ 0075-8450 ] ; 2009.
Abstract
: Gravitational lensing is strong if the distortions to the images are substantial, and weak if the distortions are small. Weak lensing of background images can be used to learn about the mass distribution in individual objects, such as galaxy clusters, but I will concentrate on weak lensing on a cosmological scale, which is usually analysed in a statistical way. Recent reviews of this area include [4, 26, 32].
Url:
DOI: 10.1007/978-3-540-44767-2_18
Links to Exploration step
ISTEX:5356761E601C87FF7F55F7369A29B52D60DC3DB1Le document en format XML
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Heavens</name><affiliation><mods:affiliation>Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK</mods:affiliation></affiliation><affiliation><mods:affiliation>E-mail: afh@roe.ac.uk</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="s">Lecture Notes in Physics</title><imprint><date>2009</date></imprint><idno type="ISSN">0075-8450</idno><idno type="eISSN">1616-6361</idno><idno type="ISSN">0075-8450</idno></series><idno type="istex">5356761E601C87FF7F55F7369A29B52D60DC3DB1</idno><idno type="DOI">10.1007/978-3-540-44767-2_18</idno><idno type="ChapterID">18</idno><idno type="ChapterID">Chap18</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0075-8450</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">: Gravitational lensing is strong if the distortions to the images are substantial, and weak if the distortions are small. 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Weak lensing of background images can be used to learn about the mass distribution in individual objects, such as galaxy clusters, but I will concentrate on weak lensing on a cosmological scale, which is usually analysed in a statistical way. Recent reviews of this area include [4, 26, 32].</Para></Abstract></ChapterHeader><NoBody></NoBody></Chapter></Part></Book></Series></Publisher></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Weak Gravitational Lensing</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>Weak Gravitational Lensing</title></titleInfo><name type="personal" displayLabel="corresp"><namePart type="given">A.</namePart><namePart type="family">Heavens</namePart><affiliation>Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK</affiliation><affiliation>E-mail: afh@roe.ac.uk</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="research-article" displayLabel="OriginalPaper"></genre><originInfo><publisher>Springer Berlin Heidelberg</publisher><place><placeTerm type="text">Berlin, Heidelberg</placeTerm></place><dateIssued encoding="w3cdtf">2008-08-23</dateIssued><copyrightDate encoding="w3cdtf">2008</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType></physicalDescription><abstract lang="en">: Gravitational lensing is strong if the distortions to the images are substantial, and weak if the distortions are small. Weak lensing of background images can be used to learn about the mass distribution in individual objects, such as galaxy clusters, but I will concentrate on weak lensing on a cosmological scale, which is usually analysed in a statistical way. 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