Strong Lensing by Galaxies
Strong lensing is a powerful tool to address three major astrophysical issues: understanding the spatial distribution of mass at kiloparsec and subkiloparsec scale, where baryons and dark matter interact to shape galaxies as we see them; determining the overall geometry, content, and kinematics of t...
Gespeichert in:
| Veröffentlicht in: | Annual review of astronomy and astrophysics 2010-01, Vol.48 (1), p.87-125 |
|---|---|
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 125 |
|---|---|
| container_issue | 1 |
| container_start_page | 87 |
| container_title | Annual review of astronomy and astrophysics |
| container_volume | 48 |
| creator | Treu, Tommaso |
| description | Strong lensing is a powerful tool to address three major astrophysical issues: understanding the spatial distribution of mass at kiloparsec and subkiloparsec scale, where baryons and dark matter interact to shape galaxies as we see them; determining the overall geometry, content, and kinematics of the Universe; and studying distant galaxies, black holes, and active nuclei that are too small or too faint to be resolved or detected with current instrumentation. After summarizing strong gravitational lensing fundamentals, I present a selection of recent important results. I conclude by discussing the exciting prospects of strong gravitational lensing in the next decade. [PUBLICATION ABSTRACT] |
| doi_str_mv | 10.1146/annurev-astro-081309-130924 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_864955581</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2128641711</sourcerecordid><originalsourceid>FETCH-LOGICAL-a504t-4d94a7eaaf8d4644cdc97d483595d3260e9954d7d12b9e5804e176d836d852853</originalsourceid><addsrcrecordid>eNpdkD9PwzAQxS0EEiXwBZgqGJgM_nPn2GJCFRSkSgzAbLmxg1KlSbEbRL89LunEcPeW9073foRcc3bLOag713VDDN_UpW3sKdNcMkP3S8ARmXAEpCC0OCYTxpSikDOn5CylFWM5j2JCLt9ysvucLkKXmqzL3XTuWvfThHROTmrXpnBx0IJ8PD2-z57p4nX-MntYUIcMthS8AVcG52rtQQFUvjKlBy3RoJdCsWAMgi89F0sTUDMIvFReyzwoNMqC3Ix3N7H_GkLa2nWTqtC2rgv9kKxWYBAxlyvI1T_nqh9il5-zJRgptQSRTfejqYp9SjHUdhObtYs7y5ndU7MHavaPmh2p2ZGa_AXiMmIH</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>749338342</pqid></control><display><type>article</type><title>Strong Lensing by Galaxies</title><source>Annual Reviews Complete A-Z List</source><creator>Treu, Tommaso</creator><creatorcontrib>Treu, Tommaso</creatorcontrib><description>Strong lensing is a powerful tool to address three major astrophysical issues: understanding the spatial distribution of mass at kiloparsec and subkiloparsec scale, where baryons and dark matter interact to shape galaxies as we see them; determining the overall geometry, content, and kinematics of the Universe; and studying distant galaxies, black holes, and active nuclei that are too small or too faint to be resolved or detected with current instrumentation. After summarizing strong gravitational lensing fundamentals, I present a selection of recent important results. I conclude by discussing the exciting prospects of strong gravitational lensing in the next decade. [PUBLICATION ABSTRACT]</description><identifier>ISSN: 0066-4146</identifier><identifier>EISSN: 1545-4282</identifier><identifier>DOI: 10.1146/annurev-astro-081309-130924</identifier><language>eng</language><publisher>Palo Alto: Annual Reviews, Inc</publisher><subject>Astrophysics ; Gravity ; Instrumentation ; Kinematics ; Spatial distribution ; Stars & galaxies</subject><ispartof>Annual review of astronomy and astrophysics, 2010-01, Vol.48 (1), p.87-125</ispartof><rights>Copyright Annual Reviews, Inc. 2010</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a504t-4d94a7eaaf8d4644cdc97d483595d3260e9954d7d12b9e5804e176d836d852853</citedby><cites>FETCH-LOGICAL-a504t-4d94a7eaaf8d4644cdc97d483595d3260e9954d7d12b9e5804e176d836d852853</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>315,782,786,4186,27933,27934</link.rule.ids></links><search><creatorcontrib>Treu, Tommaso</creatorcontrib><title>Strong Lensing by Galaxies</title><title>Annual review of astronomy and astrophysics</title><description>Strong lensing is a powerful tool to address three major astrophysical issues: understanding the spatial distribution of mass at kiloparsec and subkiloparsec scale, where baryons and dark matter interact to shape galaxies as we see them; determining the overall geometry, content, and kinematics of the Universe; and studying distant galaxies, black holes, and active nuclei that are too small or too faint to be resolved or detected with current instrumentation. After summarizing strong gravitational lensing fundamentals, I present a selection of recent important results. I conclude by discussing the exciting prospects of strong gravitational lensing in the next decade. [PUBLICATION ABSTRACT]</description><subject>Astrophysics</subject><subject>Gravity</subject><subject>Instrumentation</subject><subject>Kinematics</subject><subject>Spatial distribution</subject><subject>Stars & galaxies</subject><issn>0066-4146</issn><issn>1545-4282</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNpdkD9PwzAQxS0EEiXwBZgqGJgM_nPn2GJCFRSkSgzAbLmxg1KlSbEbRL89LunEcPeW9073foRcc3bLOag713VDDN_UpW3sKdNcMkP3S8ARmXAEpCC0OCYTxpSikDOn5CylFWM5j2JCLt9ysvucLkKXmqzL3XTuWvfThHROTmrXpnBx0IJ8PD2-z57p4nX-MntYUIcMthS8AVcG52rtQQFUvjKlBy3RoJdCsWAMgi89F0sTUDMIvFReyzwoNMqC3Ix3N7H_GkLa2nWTqtC2rgv9kKxWYBAxlyvI1T_nqh9il5-zJRgptQSRTfejqYp9SjHUdhObtYs7y5ndU7MHavaPmh2p2ZGa_AXiMmIH</recordid><startdate>20100101</startdate><enddate>20100101</enddate><creator>Treu, Tommaso</creator><general>Annual Reviews, Inc</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20100101</creationdate><title>Strong Lensing by Galaxies</title><author>Treu, Tommaso</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a504t-4d94a7eaaf8d4644cdc97d483595d3260e9954d7d12b9e5804e176d836d852853</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Astrophysics</topic><topic>Gravity</topic><topic>Instrumentation</topic><topic>Kinematics</topic><topic>Spatial distribution</topic><topic>Stars & galaxies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Treu, Tommaso</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Annual review of astronomy and astrophysics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Treu, Tommaso</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Strong Lensing by Galaxies</atitle><jtitle>Annual review of astronomy and astrophysics</jtitle><date>2010-01-01</date><risdate>2010</risdate><volume>48</volume><issue>1</issue><spage>87</spage><epage>125</epage><pages>87-125</pages><issn>0066-4146</issn><eissn>1545-4282</eissn><abstract>Strong lensing is a powerful tool to address three major astrophysical issues: understanding the spatial distribution of mass at kiloparsec and subkiloparsec scale, where baryons and dark matter interact to shape galaxies as we see them; determining the overall geometry, content, and kinematics of the Universe; and studying distant galaxies, black holes, and active nuclei that are too small or too faint to be resolved or detected with current instrumentation. After summarizing strong gravitational lensing fundamentals, I present a selection of recent important results. I conclude by discussing the exciting prospects of strong gravitational lensing in the next decade. [PUBLICATION ABSTRACT]</abstract><cop>Palo Alto</cop><pub>Annual Reviews, Inc</pub><doi>10.1146/annurev-astro-081309-130924</doi><tpages>39</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0066-4146 |
| ispartof | Annual review of astronomy and astrophysics, 2010-01, Vol.48 (1), p.87-125 |
| issn | 0066-4146 1545-4282 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_864955581 |
| source | Annual Reviews Complete A-Z List |
| subjects | Astrophysics Gravity Instrumentation Kinematics Spatial distribution Stars & galaxies |
| title | Strong Lensing by Galaxies |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-11-30T07%3A44%3A09IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Strong%20Lensing%20by%20Galaxies&rft.jtitle=Annual%20review%20of%20astronomy%20and%20astrophysics&rft.au=Treu,%20Tommaso&rft.date=2010-01-01&rft.volume=48&rft.issue=1&rft.spage=87&rft.epage=125&rft.pages=87-125&rft.issn=0066-4146&rft.eissn=1545-4282&rft_id=info:doi/10.1146/annurev-astro-081309-130924&rft_dat=%3Cproquest_cross%3E2128641711%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=749338342&rft_id=info:pmid/&rfr_iscdi=true |