Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching
We investigate the star formation properties of a large sample of ∼2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to in the Chandra COSMOS Legacy Survey in order to understand the connection between the star formation and nuclear activity. Making use of the existing multi...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal 2017-06, Vol.841 (2), p.102 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | 2 |
| container_start_page | 102 |
| container_title | The Astrophysical journal |
| container_volume | 841 |
| creator | Suh, Hyewon Civano, Francesca Hasinger, Günther Lusso, Elisabeta Lanzuisi, Giorgio Marchesi, Stefano Trakhtenbrot, Benny Allevato, Viola Cappelluti, Nico Capak, Peter L. Elvis, Martin Griffiths, Richard E. Laigle, Clotilde Lira, Paulina Riguccini, Laurie Rosario, David J. Salvato, Mara Schawinski, Kevin Vignali, Cristian |
| description | We investigate the star formation properties of a large sample of ∼2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to in the Chandra COSMOS Legacy Survey in order to understand the connection between the star formation and nuclear activity. Making use of the existing multi-wavelength photometric data available in the COSMOS field, we perform a multi-component modeling from far-infrared to near-ultraviolet using a nuclear dust torus model, a stellar population model and a starburst model of the spectral energy distributions (SEDs). Through detailed analyses of SEDs, we derive the stellar masses and the star formation rates (SFRs) of Type 2 AGN host galaxies. The stellar mass of our sample is in the range of with uncertainties of ∼0.19 dex. We find that Type 2 AGN host galaxies have, on average, similar SFRs compared to the normal star-forming galaxies with similar Mstellar and redshift ranges, suggesting no significant evidence for enhancement or quenching of star formation. This could be interpreted in a scenario, where the relative massive galaxies have already experienced substantial growth at higher redshift ( ), and grow slowly through secular fueling processes hosting moderate-luminosity AGNs. |
| doi_str_mv | 10.3847/1538-4357/aa725c |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_iop_journals_10_3847_1538_4357_aa725c</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365727317</sourcerecordid><originalsourceid>FETCH-LOGICAL-c443t-ac12a334cb67fc80aa0e8e7b1403d85fbf05a62cc7fa202c2a54d39580b6dfaa3</originalsourceid><addsrcrecordid>eNp9kU1rGzEQhkVpoW7Se46C0kvJNlp9rnszJrULTkxxCrmJsVbKyrjSVto19b_vLluSS-lpmOF5HxhehK5K8plVXN2UglUFZ0LdACgqzCs0ez69RjNCCC8kU49v0bucD-NK5_MZgodzazHFi9U9Xsfc4RUc4be3GfuAu8biZQOhTlAst7u77Q5v7BOYM9716WTPX_B9xLcnX9tgLI5utBR18icb8Pd-ODY-PF2iNw6O2b7_Oy_Qj6-3D8t1sdmuvi0Xm8JwzroCTEmBMW72UjlTEQBiK6v2JSesroTbOyJAUmOUA0qooSB4zeaiIntZOwB2gT5M3uELr7PxnTWNiSFY02lKK0WlkAP1aaIaOOo2-Z-QzjqC1-vFRvuQe02Y4opLeSpflG2Kv3qbO32IfQrDF5oyKRRVrFQDRSbKpJhzsu7ZWxI9dqPHIvRYhJ66GSLXU8TH9sX5H_zjP3BoD7ripaZDkOq2duwPBIaZTA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365727317</pqid></control><display><type>article</type><title>Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching</title><source>IOP Publishing Free Content</source><creator>Suh, Hyewon ; Civano, Francesca ; Hasinger, Günther ; Lusso, Elisabeta ; Lanzuisi, Giorgio ; Marchesi, Stefano ; Trakhtenbrot, Benny ; Allevato, Viola ; Cappelluti, Nico ; Capak, Peter L. ; Elvis, Martin ; Griffiths, Richard E. ; Laigle, Clotilde ; Lira, Paulina ; Riguccini, Laurie ; Rosario, David J. ; Salvato, Mara ; Schawinski, Kevin ; Vignali, Cristian</creator><creatorcontrib>Suh, Hyewon ; Civano, Francesca ; Hasinger, Günther ; Lusso, Elisabeta ; Lanzuisi, Giorgio ; Marchesi, Stefano ; Trakhtenbrot, Benny ; Allevato, Viola ; Cappelluti, Nico ; Capak, Peter L. ; Elvis, Martin ; Griffiths, Richard E. ; Laigle, Clotilde ; Lira, Paulina ; Riguccini, Laurie ; Rosario, David J. ; Salvato, Mara ; Schawinski, Kevin ; Vignali, Cristian</creatorcontrib><description>We investigate the star formation properties of a large sample of ∼2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to in the Chandra COSMOS Legacy Survey in order to understand the connection between the star formation and nuclear activity. Making use of the existing multi-wavelength photometric data available in the COSMOS field, we perform a multi-component modeling from far-infrared to near-ultraviolet using a nuclear dust torus model, a stellar population model and a starburst model of the spectral energy distributions (SEDs). Through detailed analyses of SEDs, we derive the stellar masses and the star formation rates (SFRs) of Type 2 AGN host galaxies. The stellar mass of our sample is in the range of with uncertainties of ∼0.19 dex. We find that Type 2 AGN host galaxies have, on average, similar SFRs compared to the normal star-forming galaxies with similar Mstellar and redshift ranges, suggesting no significant evidence for enhancement or quenching of star formation. This could be interpreted in a scenario, where the relative massive galaxies have already experienced substantial growth at higher redshift ( ), and grow slowly through secular fueling processes hosting moderate-luminosity AGNs.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/aa725c</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Active galactic nuclei ; Astrophysics ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; black hole physics ; BLACK HOLES ; COMPARATIVE EVALUATIONS ; COMPUTERIZED SIMULATION ; COSMIC DUST ; Cosmos ; ENERGY SPECTRA ; GALAXIES ; galaxies: active ; galaxies: nuclei ; GALAXY NUCLEI ; LUMINOSITY ; MASS ; Polls & surveys ; QUASARS ; quasars: general ; Quenching ; RED SHIFT ; Sciences of the Universe ; Star & galaxy formation ; Star formation ; STARS ; Stars & galaxies ; Stellar mass ; Stellar models ; Toruses ; ULTRAVIOLET RADIATION ; UNIVERSE</subject><ispartof>The Astrophysical journal, 2017-06, Vol.841 (2), p.102</ispartof><rights>2017. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Jun 01, 2017</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c443t-ac12a334cb67fc80aa0e8e7b1403d85fbf05a62cc7fa202c2a54d39580b6dfaa3</citedby><cites>FETCH-LOGICAL-c443t-ac12a334cb67fc80aa0e8e7b1403d85fbf05a62cc7fa202c2a54d39580b6dfaa3</cites><orcidid>0000-0001-7116-9303 ; 0000-0002-0001-3587 ; 0000-0002-2536-1633 ; 0000-0001-5464-0888 ; 0000-0003-0083-1157 ; 0000-0001-5060-1398 ; 0000-0001-5544-0749 ; 0000-0002-1697-186X ; 0000-0001-9094-0984 ; 0000-0002-3683-7297 ; 0000-0002-0797-0646 ; 0000-0002-8853-9611 ; 0000-0001-7232-5152</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/aa725c/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,777,781,882,27905,27906,38871,53848</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/aa725c$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://insu.hal.science/insu-03747466$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/22872656$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Suh, Hyewon</creatorcontrib><creatorcontrib>Civano, Francesca</creatorcontrib><creatorcontrib>Hasinger, Günther</creatorcontrib><creatorcontrib>Lusso, Elisabeta</creatorcontrib><creatorcontrib>Lanzuisi, Giorgio</creatorcontrib><creatorcontrib>Marchesi, Stefano</creatorcontrib><creatorcontrib>Trakhtenbrot, Benny</creatorcontrib><creatorcontrib>Allevato, Viola</creatorcontrib><creatorcontrib>Cappelluti, Nico</creatorcontrib><creatorcontrib>Capak, Peter L.</creatorcontrib><creatorcontrib>Elvis, Martin</creatorcontrib><creatorcontrib>Griffiths, Richard E.</creatorcontrib><creatorcontrib>Laigle, Clotilde</creatorcontrib><creatorcontrib>Lira, Paulina</creatorcontrib><creatorcontrib>Riguccini, Laurie</creatorcontrib><creatorcontrib>Rosario, David J.</creatorcontrib><creatorcontrib>Salvato, Mara</creatorcontrib><creatorcontrib>Schawinski, Kevin</creatorcontrib><creatorcontrib>Vignali, Cristian</creatorcontrib><title>Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>We investigate the star formation properties of a large sample of ∼2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to in the Chandra COSMOS Legacy Survey in order to understand the connection between the star formation and nuclear activity. Making use of the existing multi-wavelength photometric data available in the COSMOS field, we perform a multi-component modeling from far-infrared to near-ultraviolet using a nuclear dust torus model, a stellar population model and a starburst model of the spectral energy distributions (SEDs). Through detailed analyses of SEDs, we derive the stellar masses and the star formation rates (SFRs) of Type 2 AGN host galaxies. The stellar mass of our sample is in the range of with uncertainties of ∼0.19 dex. We find that Type 2 AGN host galaxies have, on average, similar SFRs compared to the normal star-forming galaxies with similar Mstellar and redshift ranges, suggesting no significant evidence for enhancement or quenching of star formation. This could be interpreted in a scenario, where the relative massive galaxies have already experienced substantial growth at higher redshift ( ), and grow slowly through secular fueling processes hosting moderate-luminosity AGNs.</description><subject>Active galactic nuclei</subject><subject>Astrophysics</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>black hole physics</subject><subject>BLACK HOLES</subject><subject>COMPARATIVE EVALUATIONS</subject><subject>COMPUTERIZED SIMULATION</subject><subject>COSMIC DUST</subject><subject>Cosmos</subject><subject>ENERGY SPECTRA</subject><subject>GALAXIES</subject><subject>galaxies: active</subject><subject>galaxies: nuclei</subject><subject>GALAXY NUCLEI</subject><subject>LUMINOSITY</subject><subject>MASS</subject><subject>Polls & surveys</subject><subject>QUASARS</subject><subject>quasars: general</subject><subject>Quenching</subject><subject>RED SHIFT</subject><subject>Sciences of the Universe</subject><subject>Star & galaxy formation</subject><subject>Star formation</subject><subject>STARS</subject><subject>Stars & galaxies</subject><subject>Stellar mass</subject><subject>Stellar models</subject><subject>Toruses</subject><subject>ULTRAVIOLET RADIATION</subject><subject>UNIVERSE</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp9kU1rGzEQhkVpoW7Se46C0kvJNlp9rnszJrULTkxxCrmJsVbKyrjSVto19b_vLluSS-lpmOF5HxhehK5K8plVXN2UglUFZ0LdACgqzCs0ez69RjNCCC8kU49v0bucD-NK5_MZgodzazHFi9U9Xsfc4RUc4be3GfuAu8biZQOhTlAst7u77Q5v7BOYM9716WTPX_B9xLcnX9tgLI5utBR18icb8Pd-ODY-PF2iNw6O2b7_Oy_Qj6-3D8t1sdmuvi0Xm8JwzroCTEmBMW72UjlTEQBiK6v2JSesroTbOyJAUmOUA0qooSB4zeaiIntZOwB2gT5M3uELr7PxnTWNiSFY02lKK0WlkAP1aaIaOOo2-Z-QzjqC1-vFRvuQe02Y4opLeSpflG2Kv3qbO32IfQrDF5oyKRRVrFQDRSbKpJhzsu7ZWxI9dqPHIvRYhJ66GSLXU8TH9sX5H_zjP3BoD7ripaZDkOq2duwPBIaZTA</recordid><startdate>20170601</startdate><enddate>20170601</enddate><creator>Suh, Hyewon</creator><creator>Civano, Francesca</creator><creator>Hasinger, Günther</creator><creator>Lusso, Elisabeta</creator><creator>Lanzuisi, Giorgio</creator><creator>Marchesi, Stefano</creator><creator>Trakhtenbrot, Benny</creator><creator>Allevato, Viola</creator><creator>Cappelluti, Nico</creator><creator>Capak, Peter L.</creator><creator>Elvis, Martin</creator><creator>Griffiths, Richard E.</creator><creator>Laigle, Clotilde</creator><creator>Lira, Paulina</creator><creator>Riguccini, Laurie</creator><creator>Rosario, David J.</creator><creator>Salvato, Mara</creator><creator>Schawinski, Kevin</creator><creator>Vignali, Cristian</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><general>American Astronomical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>1XC</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0001-7116-9303</orcidid><orcidid>https://orcid.org/0000-0002-0001-3587</orcidid><orcidid>https://orcid.org/0000-0002-2536-1633</orcidid><orcidid>https://orcid.org/0000-0001-5464-0888</orcidid><orcidid>https://orcid.org/0000-0003-0083-1157</orcidid><orcidid>https://orcid.org/0000-0001-5060-1398</orcidid><orcidid>https://orcid.org/0000-0001-5544-0749</orcidid><orcidid>https://orcid.org/0000-0002-1697-186X</orcidid><orcidid>https://orcid.org/0000-0001-9094-0984</orcidid><orcidid>https://orcid.org/0000-0002-3683-7297</orcidid><orcidid>https://orcid.org/0000-0002-0797-0646</orcidid><orcidid>https://orcid.org/0000-0002-8853-9611</orcidid><orcidid>https://orcid.org/0000-0001-7232-5152</orcidid></search><sort><creationdate>20170601</creationdate><title>Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching</title><author>Suh, Hyewon ; Civano, Francesca ; Hasinger, Günther ; Lusso, Elisabeta ; Lanzuisi, Giorgio ; Marchesi, Stefano ; Trakhtenbrot, Benny ; Allevato, Viola ; Cappelluti, Nico ; Capak, Peter L. ; Elvis, Martin ; Griffiths, Richard E. ; Laigle, Clotilde ; Lira, Paulina ; Riguccini, Laurie ; Rosario, David J. ; Salvato, Mara ; Schawinski, Kevin ; Vignali, Cristian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c443t-ac12a334cb67fc80aa0e8e7b1403d85fbf05a62cc7fa202c2a54d39580b6dfaa3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Active galactic nuclei</topic><topic>Astrophysics</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>black hole physics</topic><topic>BLACK HOLES</topic><topic>COMPARATIVE EVALUATIONS</topic><topic>COMPUTERIZED SIMULATION</topic><topic>COSMIC DUST</topic><topic>Cosmos</topic><topic>ENERGY SPECTRA</topic><topic>GALAXIES</topic><topic>galaxies: active</topic><topic>galaxies: nuclei</topic><topic>GALAXY NUCLEI</topic><topic>LUMINOSITY</topic><topic>MASS</topic><topic>Polls & surveys</topic><topic>QUASARS</topic><topic>quasars: general</topic><topic>Quenching</topic><topic>RED SHIFT</topic><topic>Sciences of the Universe</topic><topic>Star & galaxy formation</topic><topic>Star formation</topic><topic>STARS</topic><topic>Stars & galaxies</topic><topic>Stellar mass</topic><topic>Stellar models</topic><topic>Toruses</topic><topic>ULTRAVIOLET RADIATION</topic><topic>UNIVERSE</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Suh, Hyewon</creatorcontrib><creatorcontrib>Civano, Francesca</creatorcontrib><creatorcontrib>Hasinger, Günther</creatorcontrib><creatorcontrib>Lusso, Elisabeta</creatorcontrib><creatorcontrib>Lanzuisi, Giorgio</creatorcontrib><creatorcontrib>Marchesi, Stefano</creatorcontrib><creatorcontrib>Trakhtenbrot, Benny</creatorcontrib><creatorcontrib>Allevato, Viola</creatorcontrib><creatorcontrib>Cappelluti, Nico</creatorcontrib><creatorcontrib>Capak, Peter L.</creatorcontrib><creatorcontrib>Elvis, Martin</creatorcontrib><creatorcontrib>Griffiths, Richard E.</creatorcontrib><creatorcontrib>Laigle, Clotilde</creatorcontrib><creatorcontrib>Lira, Paulina</creatorcontrib><creatorcontrib>Riguccini, Laurie</creatorcontrib><creatorcontrib>Rosario, David J.</creatorcontrib><creatorcontrib>Salvato, Mara</creatorcontrib><creatorcontrib>Schawinski, Kevin</creatorcontrib><creatorcontrib>Vignali, Cristian</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><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Suh, Hyewon</au><au>Civano, Francesca</au><au>Hasinger, Günther</au><au>Lusso, Elisabeta</au><au>Lanzuisi, Giorgio</au><au>Marchesi, Stefano</au><au>Trakhtenbrot, Benny</au><au>Allevato, Viola</au><au>Cappelluti, Nico</au><au>Capak, Peter L.</au><au>Elvis, Martin</au><au>Griffiths, Richard E.</au><au>Laigle, Clotilde</au><au>Lira, Paulina</au><au>Riguccini, Laurie</au><au>Rosario, David J.</au><au>Salvato, Mara</au><au>Schawinski, Kevin</au><au>Vignali, Cristian</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2017-06-01</date><risdate>2017</risdate><volume>841</volume><issue>2</issue><spage>102</spage><pages>102-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>We investigate the star formation properties of a large sample of ∼2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to in the Chandra COSMOS Legacy Survey in order to understand the connection between the star formation and nuclear activity. Making use of the existing multi-wavelength photometric data available in the COSMOS field, we perform a multi-component modeling from far-infrared to near-ultraviolet using a nuclear dust torus model, a stellar population model and a starburst model of the spectral energy distributions (SEDs). Through detailed analyses of SEDs, we derive the stellar masses and the star formation rates (SFRs) of Type 2 AGN host galaxies. The stellar mass of our sample is in the range of with uncertainties of ∼0.19 dex. We find that Type 2 AGN host galaxies have, on average, similar SFRs compared to the normal star-forming galaxies with similar Mstellar and redshift ranges, suggesting no significant evidence for enhancement or quenching of star formation. This could be interpreted in a scenario, where the relative massive galaxies have already experienced substantial growth at higher redshift ( ), and grow slowly through secular fueling processes hosting moderate-luminosity AGNs.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/aa725c</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0001-7116-9303</orcidid><orcidid>https://orcid.org/0000-0002-0001-3587</orcidid><orcidid>https://orcid.org/0000-0002-2536-1633</orcidid><orcidid>https://orcid.org/0000-0001-5464-0888</orcidid><orcidid>https://orcid.org/0000-0003-0083-1157</orcidid><orcidid>https://orcid.org/0000-0001-5060-1398</orcidid><orcidid>https://orcid.org/0000-0001-5544-0749</orcidid><orcidid>https://orcid.org/0000-0002-1697-186X</orcidid><orcidid>https://orcid.org/0000-0001-9094-0984</orcidid><orcidid>https://orcid.org/0000-0002-3683-7297</orcidid><orcidid>https://orcid.org/0000-0002-0797-0646</orcidid><orcidid>https://orcid.org/0000-0002-8853-9611</orcidid><orcidid>https://orcid.org/0000-0001-7232-5152</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0004-637X |
| ispartof | The Astrophysical journal, 2017-06, Vol.841 (2), p.102 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_iop_journals_10_3847_1538_4357_aa725c |
| source | IOP Publishing Free Content |
| subjects | Active galactic nuclei Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY black hole physics BLACK HOLES COMPARATIVE EVALUATIONS COMPUTERIZED SIMULATION COSMIC DUST Cosmos ENERGY SPECTRA GALAXIES galaxies: active galaxies: nuclei GALAXY NUCLEI LUMINOSITY MASS Polls & surveys QUASARS quasars: general Quenching RED SHIFT Sciences of the Universe Star & galaxy formation Star formation STARS Stars & galaxies Stellar mass Stellar models Toruses ULTRAVIOLET RADIATION UNIVERSE |
| title | Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-18T02%3A13%3A31IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Type%202%20AGN%20Host%20Galaxies%20in%20the%20Chandra-COSMOS%20Legacy%20Survey:%20No%20Evidence%20of%20AGN-driven%20Quenching&rft.jtitle=The%20Astrophysical%20journal&rft.au=Suh,%20Hyewon&rft.date=2017-06-01&rft.volume=841&rft.issue=2&rft.spage=102&rft.pages=102-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/aa725c&rft_dat=%3Cproquest_O3W%3E2365727317%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2365727317&rft_id=info:pmid/&rfr_iscdi=true |