AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey
Multiwavelength surveys covering large sky volumes are necessary to obtain an accurate census of rare objects such as high-luminosity and/or high-redshift active galactic nuclei (AGNs). Stripe 82X is a 31.3 X-ray survey with Chandra and XMM-Newton observations overlapping the legacy Sloan Digital Sk...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal 2017-11, Vol.850 (1), p.66 |
|---|---|
| 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 | 1 |
| container_start_page | 66 |
| container_title | The Astrophysical journal |
| container_volume | 850 |
| creator | Ananna, Tonima Tasnim Salvato, Mara LaMassa, Stephanie Urry, C. Megan Cappelluti, Nico Cardamone, Carolin Civano, Francesca Farrah, Duncan Gilfanov, Marat Glikman, Eilat Hamilton, Mark Kirkpatrick, Allison Lanzuisi, Giorgio Marchesi, Stefano Merloni, Andrea Nandra, Kirpal Natarajan, Priyamvada Richards, Gordon T. Timlin, John |
| description | Multiwavelength surveys covering large sky volumes are necessary to obtain an accurate census of rare objects such as high-luminosity and/or high-redshift active galactic nuclei (AGNs). Stripe 82X is a 31.3 X-ray survey with Chandra and XMM-Newton observations overlapping the legacy Sloan Digital Sky Survey Stripe 82 field, which has a rich investment of multiwavelength coverage from the ultraviolet to the radio. The wide-area nature of this survey presents new challenges for photometric redshifts for AGNs compared to previous work on narrow-deep fields because it probes different populations of objects that need to be identified and represented in the library of templates. Here we present an updated X-ray plus multiwavelength matched catalog, including Spitzer counterparts, and estimated photometric redshifts for 5961 (96% of a total of 6181) X-ray sources that have a normalized median absolute deviation, , and an outlier fraction, = 13.7%. The populations found in this survey and the template libraries used for photometric redshifts provide important guiding principles for upcoming large-area surveys such as eROSITA and 3XMM (in X-ray) and the Large Synoptic Survey Telescope (optical). |
| doi_str_mv | 10.3847/1538-4357/aa937d |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_crossref_primary_10_3847_1538_4357_aa937d</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365858954</sourcerecordid><originalsourceid>FETCH-LOGICAL-c416t-696f197e5e595fee4ffb5b0c50c58690eea427d408b5b4ad901712de348c061b3</originalsourceid><addsrcrecordid>eNp1kFFLwzAUhYMoOKfvPgZ8tS5pkzbxbQw3haFjm7C3kLW3rmNbatIO--9N6VBfhAuXezjnu3AQuqXkIRIsGVAeiYBFPBloLaMkO0O9H-kc9QghLIijZHWJrpzbtmcoZQ99DSeveGbKeqerwhwcLg54qu0HBEezq_eAV8FcN3hR2yM07hHPNqYye6hskeI5ZG5T5JXD-pD9geBlU4LDY1N72fOqDeCFT5SARbg6sa7RRa53Dm5Ou4_ex0_L0XMwfZu8jIbTIGU0roJYxjmVCXDgkucALM_XfE1S7kfEkgBoFiYZI8LLTGeS0ISGGURMpCSm66iP7jpuac1nDa5SW1Pbg3-pwijmggvJmXeRzpVa45yFXJW22GvbKEpU269qy1Rtmarr10fuu0hhyl_mv_ZvvB98XQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365858954</pqid></control><display><type>article</type><title>AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey</title><source>IOP Publishing Free Content</source><creator>Ananna, Tonima Tasnim ; Salvato, Mara ; LaMassa, Stephanie ; Urry, C. Megan ; Cappelluti, Nico ; Cardamone, Carolin ; Civano, Francesca ; Farrah, Duncan ; Gilfanov, Marat ; Glikman, Eilat ; Hamilton, Mark ; Kirkpatrick, Allison ; Lanzuisi, Giorgio ; Marchesi, Stefano ; Merloni, Andrea ; Nandra, Kirpal ; Natarajan, Priyamvada ; Richards, Gordon T. ; Timlin, John</creator><creatorcontrib>Ananna, Tonima Tasnim ; Salvato, Mara ; LaMassa, Stephanie ; Urry, C. Megan ; Cappelluti, Nico ; Cardamone, Carolin ; Civano, Francesca ; Farrah, Duncan ; Gilfanov, Marat ; Glikman, Eilat ; Hamilton, Mark ; Kirkpatrick, Allison ; Lanzuisi, Giorgio ; Marchesi, Stefano ; Merloni, Andrea ; Nandra, Kirpal ; Natarajan, Priyamvada ; Richards, Gordon T. ; Timlin, John</creatorcontrib><description>Multiwavelength surveys covering large sky volumes are necessary to obtain an accurate census of rare objects such as high-luminosity and/or high-redshift active galactic nuclei (AGNs). Stripe 82X is a 31.3 X-ray survey with Chandra and XMM-Newton observations overlapping the legacy Sloan Digital Sky Survey Stripe 82 field, which has a rich investment of multiwavelength coverage from the ultraviolet to the radio. The wide-area nature of this survey presents new challenges for photometric redshifts for AGNs compared to previous work on narrow-deep fields because it probes different populations of objects that need to be identified and represented in the library of templates. Here we present an updated X-ray plus multiwavelength matched catalog, including Spitzer counterparts, and estimated photometric redshifts for 5961 (96% of a total of 6181) X-ray sources that have a normalized median absolute deviation, , and an outlier fraction, = 13.7%. The populations found in this survey and the template libraries used for photometric redshifts provide important guiding principles for upcoming large-area surveys such as eROSITA and 3XMM (in X-ray) and the Large Synoptic Survey Telescope (optical).</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/aa937d</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Active galactic nuclei ; Astrophysics ; Luminosity ; Outliers (statistics) ; Photometry ; Populations ; quasars: absorption lines ; quasars: emission lines ; quasars: general ; Red shift ; Sky surveys (astronomy) ; techniques: photometric ; techniques: spectroscopic ; X ray sources ; XMM (spacecraft)</subject><ispartof>The Astrophysical journal, 2017-11, Vol.850 (1), p.66</ispartof><rights>2017. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Nov 20, 2017</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c416t-696f197e5e595fee4ffb5b0c50c58690eea427d408b5b4ad901712de348c061b3</citedby><cites>FETCH-LOGICAL-c416t-696f197e5e595fee4ffb5b0c50c58690eea427d408b5b4ad901712de348c061b3</cites><orcidid>0000-0002-5907-3330 ; 0000-0001-7116-9303 ; 0000-0003-1748-2010 ; 0000-0001-9094-0984 ; 0000-0001-8131-1801 ; 0000-0002-0745-9792 ; 0000-0002-1306-1545 ; 0000-0003-4608-6340 ; 0000-0002-1697-186X ; 0000-0001-5544-0749 ; 0000-0003-0489-3750 ; 0000-0002-5554-8896 ; 0000-0002-7150-9192 ; 0000-0002-1061-1804</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/aa937d/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>315,781,785,27926,27927,38892,53869</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/aa937d$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc></links><search><creatorcontrib>Ananna, Tonima Tasnim</creatorcontrib><creatorcontrib>Salvato, Mara</creatorcontrib><creatorcontrib>LaMassa, Stephanie</creatorcontrib><creatorcontrib>Urry, C. Megan</creatorcontrib><creatorcontrib>Cappelluti, Nico</creatorcontrib><creatorcontrib>Cardamone, Carolin</creatorcontrib><creatorcontrib>Civano, Francesca</creatorcontrib><creatorcontrib>Farrah, Duncan</creatorcontrib><creatorcontrib>Gilfanov, Marat</creatorcontrib><creatorcontrib>Glikman, Eilat</creatorcontrib><creatorcontrib>Hamilton, Mark</creatorcontrib><creatorcontrib>Kirkpatrick, Allison</creatorcontrib><creatorcontrib>Lanzuisi, Giorgio</creatorcontrib><creatorcontrib>Marchesi, Stefano</creatorcontrib><creatorcontrib>Merloni, Andrea</creatorcontrib><creatorcontrib>Nandra, Kirpal</creatorcontrib><creatorcontrib>Natarajan, Priyamvada</creatorcontrib><creatorcontrib>Richards, Gordon T.</creatorcontrib><creatorcontrib>Timlin, John</creatorcontrib><title>AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>Multiwavelength surveys covering large sky volumes are necessary to obtain an accurate census of rare objects such as high-luminosity and/or high-redshift active galactic nuclei (AGNs). Stripe 82X is a 31.3 X-ray survey with Chandra and XMM-Newton observations overlapping the legacy Sloan Digital Sky Survey Stripe 82 field, which has a rich investment of multiwavelength coverage from the ultraviolet to the radio. The wide-area nature of this survey presents new challenges for photometric redshifts for AGNs compared to previous work on narrow-deep fields because it probes different populations of objects that need to be identified and represented in the library of templates. Here we present an updated X-ray plus multiwavelength matched catalog, including Spitzer counterparts, and estimated photometric redshifts for 5961 (96% of a total of 6181) X-ray sources that have a normalized median absolute deviation, , and an outlier fraction, = 13.7%. The populations found in this survey and the template libraries used for photometric redshifts provide important guiding principles for upcoming large-area surveys such as eROSITA and 3XMM (in X-ray) and the Large Synoptic Survey Telescope (optical).</description><subject>Active galactic nuclei</subject><subject>Astrophysics</subject><subject>Luminosity</subject><subject>Outliers (statistics)</subject><subject>Photometry</subject><subject>Populations</subject><subject>quasars: absorption lines</subject><subject>quasars: emission lines</subject><subject>quasars: general</subject><subject>Red shift</subject><subject>Sky surveys (astronomy)</subject><subject>techniques: photometric</subject><subject>techniques: spectroscopic</subject><subject>X ray sources</subject><subject>XMM (spacecraft)</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp1kFFLwzAUhYMoOKfvPgZ8tS5pkzbxbQw3haFjm7C3kLW3rmNbatIO--9N6VBfhAuXezjnu3AQuqXkIRIsGVAeiYBFPBloLaMkO0O9H-kc9QghLIijZHWJrpzbtmcoZQ99DSeveGbKeqerwhwcLg54qu0HBEezq_eAV8FcN3hR2yM07hHPNqYye6hskeI5ZG5T5JXD-pD9geBlU4LDY1N72fOqDeCFT5SARbg6sa7RRa53Dm5Ou4_ex0_L0XMwfZu8jIbTIGU0roJYxjmVCXDgkucALM_XfE1S7kfEkgBoFiYZI8LLTGeS0ISGGURMpCSm66iP7jpuac1nDa5SW1Pbg3-pwijmggvJmXeRzpVa45yFXJW22GvbKEpU269qy1Rtmarr10fuu0hhyl_mv_ZvvB98XQ</recordid><startdate>20171120</startdate><enddate>20171120</enddate><creator>Ananna, Tonima Tasnim</creator><creator>Salvato, Mara</creator><creator>LaMassa, Stephanie</creator><creator>Urry, C. Megan</creator><creator>Cappelluti, Nico</creator><creator>Cardamone, Carolin</creator><creator>Civano, Francesca</creator><creator>Farrah, Duncan</creator><creator>Gilfanov, Marat</creator><creator>Glikman, Eilat</creator><creator>Hamilton, Mark</creator><creator>Kirkpatrick, Allison</creator><creator>Lanzuisi, Giorgio</creator><creator>Marchesi, Stefano</creator><creator>Merloni, Andrea</creator><creator>Nandra, Kirpal</creator><creator>Natarajan, Priyamvada</creator><creator>Richards, Gordon T.</creator><creator>Timlin, John</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-5907-3330</orcidid><orcidid>https://orcid.org/0000-0001-7116-9303</orcidid><orcidid>https://orcid.org/0000-0003-1748-2010</orcidid><orcidid>https://orcid.org/0000-0001-9094-0984</orcidid><orcidid>https://orcid.org/0000-0001-8131-1801</orcidid><orcidid>https://orcid.org/0000-0002-0745-9792</orcidid><orcidid>https://orcid.org/0000-0002-1306-1545</orcidid><orcidid>https://orcid.org/0000-0003-4608-6340</orcidid><orcidid>https://orcid.org/0000-0002-1697-186X</orcidid><orcidid>https://orcid.org/0000-0001-5544-0749</orcidid><orcidid>https://orcid.org/0000-0003-0489-3750</orcidid><orcidid>https://orcid.org/0000-0002-5554-8896</orcidid><orcidid>https://orcid.org/0000-0002-7150-9192</orcidid><orcidid>https://orcid.org/0000-0002-1061-1804</orcidid></search><sort><creationdate>20171120</creationdate><title>AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey</title><author>Ananna, Tonima Tasnim ; Salvato, Mara ; LaMassa, Stephanie ; Urry, C. Megan ; Cappelluti, Nico ; Cardamone, Carolin ; Civano, Francesca ; Farrah, Duncan ; Gilfanov, Marat ; Glikman, Eilat ; Hamilton, Mark ; Kirkpatrick, Allison ; Lanzuisi, Giorgio ; Marchesi, Stefano ; Merloni, Andrea ; Nandra, Kirpal ; Natarajan, Priyamvada ; Richards, Gordon T. ; Timlin, John</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c416t-696f197e5e595fee4ffb5b0c50c58690eea427d408b5b4ad901712de348c061b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Active galactic nuclei</topic><topic>Astrophysics</topic><topic>Luminosity</topic><topic>Outliers (statistics)</topic><topic>Photometry</topic><topic>Populations</topic><topic>quasars: absorption lines</topic><topic>quasars: emission lines</topic><topic>quasars: general</topic><topic>Red shift</topic><topic>Sky surveys (astronomy)</topic><topic>techniques: photometric</topic><topic>techniques: spectroscopic</topic><topic>X ray sources</topic><topic>XMM (spacecraft)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ananna, Tonima Tasnim</creatorcontrib><creatorcontrib>Salvato, Mara</creatorcontrib><creatorcontrib>LaMassa, Stephanie</creatorcontrib><creatorcontrib>Urry, C. Megan</creatorcontrib><creatorcontrib>Cappelluti, Nico</creatorcontrib><creatorcontrib>Cardamone, Carolin</creatorcontrib><creatorcontrib>Civano, Francesca</creatorcontrib><creatorcontrib>Farrah, Duncan</creatorcontrib><creatorcontrib>Gilfanov, Marat</creatorcontrib><creatorcontrib>Glikman, Eilat</creatorcontrib><creatorcontrib>Hamilton, Mark</creatorcontrib><creatorcontrib>Kirkpatrick, Allison</creatorcontrib><creatorcontrib>Lanzuisi, Giorgio</creatorcontrib><creatorcontrib>Marchesi, Stefano</creatorcontrib><creatorcontrib>Merloni, Andrea</creatorcontrib><creatorcontrib>Nandra, Kirpal</creatorcontrib><creatorcontrib>Natarajan, Priyamvada</creatorcontrib><creatorcontrib>Richards, Gordon T.</creatorcontrib><creatorcontrib>Timlin, John</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>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Ananna, Tonima Tasnim</au><au>Salvato, Mara</au><au>LaMassa, Stephanie</au><au>Urry, C. Megan</au><au>Cappelluti, Nico</au><au>Cardamone, Carolin</au><au>Civano, Francesca</au><au>Farrah, Duncan</au><au>Gilfanov, Marat</au><au>Glikman, Eilat</au><au>Hamilton, Mark</au><au>Kirkpatrick, Allison</au><au>Lanzuisi, Giorgio</au><au>Marchesi, Stefano</au><au>Merloni, Andrea</au><au>Nandra, Kirpal</au><au>Natarajan, Priyamvada</au><au>Richards, Gordon T.</au><au>Timlin, John</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2017-11-20</date><risdate>2017</risdate><volume>850</volume><issue>1</issue><spage>66</spage><pages>66-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Multiwavelength surveys covering large sky volumes are necessary to obtain an accurate census of rare objects such as high-luminosity and/or high-redshift active galactic nuclei (AGNs). Stripe 82X is a 31.3 X-ray survey with Chandra and XMM-Newton observations overlapping the legacy Sloan Digital Sky Survey Stripe 82 field, which has a rich investment of multiwavelength coverage from the ultraviolet to the radio. The wide-area nature of this survey presents new challenges for photometric redshifts for AGNs compared to previous work on narrow-deep fields because it probes different populations of objects that need to be identified and represented in the library of templates. Here we present an updated X-ray plus multiwavelength matched catalog, including Spitzer counterparts, and estimated photometric redshifts for 5961 (96% of a total of 6181) X-ray sources that have a normalized median absolute deviation, , and an outlier fraction, = 13.7%. The populations found in this survey and the template libraries used for photometric redshifts provide important guiding principles for upcoming large-area surveys such as eROSITA and 3XMM (in X-ray) and the Large Synoptic Survey Telescope (optical).</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/aa937d</doi><tpages>26</tpages><orcidid>https://orcid.org/0000-0002-5907-3330</orcidid><orcidid>https://orcid.org/0000-0001-7116-9303</orcidid><orcidid>https://orcid.org/0000-0003-1748-2010</orcidid><orcidid>https://orcid.org/0000-0001-9094-0984</orcidid><orcidid>https://orcid.org/0000-0001-8131-1801</orcidid><orcidid>https://orcid.org/0000-0002-0745-9792</orcidid><orcidid>https://orcid.org/0000-0002-1306-1545</orcidid><orcidid>https://orcid.org/0000-0003-4608-6340</orcidid><orcidid>https://orcid.org/0000-0002-1697-186X</orcidid><orcidid>https://orcid.org/0000-0001-5544-0749</orcidid><orcidid>https://orcid.org/0000-0003-0489-3750</orcidid><orcidid>https://orcid.org/0000-0002-5554-8896</orcidid><orcidid>https://orcid.org/0000-0002-7150-9192</orcidid><orcidid>https://orcid.org/0000-0002-1061-1804</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0004-637X |
| ispartof | The Astrophysical journal, 2017-11, Vol.850 (1), p.66 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_crossref_primary_10_3847_1538_4357_aa937d |
| source | IOP Publishing Free Content |
| subjects | Active galactic nuclei Astrophysics Luminosity Outliers (statistics) Photometry Populations quasars: absorption lines quasars: emission lines quasars: general Red shift Sky surveys (astronomy) techniques: photometric techniques: spectroscopic X ray sources XMM (spacecraft) |
| title | AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-18T05%3A01%3A58IST&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=AGN%20Populations%20in%20Large-volume%20X-Ray%20Surveys:%20Photometric%20Redshifts%20and%20Population%20Types%20Found%20in%20the%20Stripe%2082X%20Survey&rft.jtitle=The%20Astrophysical%20journal&rft.au=Ananna,%20Tonima%20Tasnim&rft.date=2017-11-20&rft.volume=850&rft.issue=1&rft.spage=66&rft.pages=66-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/aa937d&rft_dat=%3Cproquest_O3W%3E2365858954%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=2365858954&rft_id=info:pmid/&rfr_iscdi=true |