A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16
We present a catalog of continuum and emission-line properties for 750,414 broad-line quasars included in the Sloan Digital Sky Survey Data Release 16 quasar catalog (DR16Q), measured from optical spectroscopy. These quasars cover broad ranges in redshift (0.1 ≲ z ≲ 6) and luminosity (44 ≲ log( L bo...
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description | We present a catalog of continuum and emission-line properties for 750,414 broad-line quasars included in the Sloan Digital Sky Survey Data Release 16 quasar catalog (DR16Q), measured from optical spectroscopy. These quasars cover broad ranges in redshift (0.1 ≲
z
≲ 6) and luminosity (44 ≲ log(
L
bol
/erg s
−1
) ≲ 48), and probe lower luminosities than an earlier compilation of SDSS DR7 quasars. Derived physical quantities such as single-epoch virial black hole masses and bolometric luminosities are also included in this catalog. We present improved systemic redshifts and realistic redshift uncertainties for DR16Q quasars using the measured line peaks and correcting for velocity shifts of various lines with respect to the systemic velocity. About 1%, 1.4%, and 11% of the original DR16Q redshifts deviate from the systemic redshifts by ∣Δ
V
∣ > 1500 km s
−1
, ∣Δ
V
∣ ∈ [1000, 1500] km s
−1
, and ∣Δ
V
∣ ∈ [500, 1000] km s
−1
, respectively; about 1900 DR16Q redshifts were catastrophically wrong (∣Δ
V
∣ > 10,000 km s
−1
). We demonstrate the utility of this data product in quantifying the spectral diversity and correlations among physical properties of quasars with large statistical samples. |
doi_str_mv | 10.3847/1538-4365/ac9ead |
format | Article |
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z
≲ 6) and luminosity (44 ≲ log(
L
bol
/erg s
−1
) ≲ 48), and probe lower luminosities than an earlier compilation of SDSS DR7 quasars. Derived physical quantities such as single-epoch virial black hole masses and bolometric luminosities are also included in this catalog. We present improved systemic redshifts and realistic redshift uncertainties for DR16Q quasars using the measured line peaks and correcting for velocity shifts of various lines with respect to the systemic velocity. About 1%, 1.4%, and 11% of the original DR16Q redshifts deviate from the systemic redshifts by ∣Δ
V
∣ > 1500 km s
−1
, ∣Δ
V
∣ ∈ [1000, 1500] km s
−1
, and ∣Δ
V
∣ ∈ [500, 1000] km s
−1
, respectively; about 1900 DR16Q redshifts were catastrophically wrong (∣Δ
V
∣ > 10,000 km s
−1
). We demonstrate the utility of this data product in quantifying the spectral diversity and correlations among physical properties of quasars with large statistical samples.</description><identifier>ISSN: 0067-0049</identifier><identifier>EISSN: 1538-4365</identifier><identifier>DOI: 10.3847/1538-4365/ac9ead</identifier><language>eng</language><publisher>Saskatoon: The American Astronomical Society</publisher><subject>Astronomy & Astrophysics ; Black holes ; Luminosity ; Physical properties ; Quasars ; Red shift ; Sky surveys (astronomy) ; Spectroscopy ; Statistical analysis ; Surveys ; Velocity</subject><ispartof>The Astrophysical journal. Supplement series, 2022-12, Vol.263 (2), p.42</ispartof><rights>2022. The Author(s). Published by the American Astronomical Society.</rights><rights>2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c407t-f12bdc9fff0ba54f2af2d604c598b95b48915b52f8c6cf942b4a8d0521924d53</citedby><cites>FETCH-LOGICAL-c407t-f12bdc9fff0ba54f2af2d604c598b95b48915b52f8c6cf942b4a8d0521924d53</cites><orcidid>0000-0003-1659-7035 ; 0000-0003-4202-1232 ; 0000000316597035 ; 0000000342021232</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4365/ac9ead/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>230,314,776,780,860,881,27901,27902,38845,38867,53815,53842</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/2425061$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Wu, Qiaoya</creatorcontrib><creatorcontrib>Shen, Yue</creatorcontrib><creatorcontrib>US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)</creatorcontrib><title>A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16</title><title>The Astrophysical journal. Supplement series</title><addtitle>APJS</addtitle><addtitle>Astrophys. J. Suppl</addtitle><description>We present a catalog of continuum and emission-line properties for 750,414 broad-line quasars included in the Sloan Digital Sky Survey Data Release 16 quasar catalog (DR16Q), measured from optical spectroscopy. These quasars cover broad ranges in redshift (0.1 ≲
z
≲ 6) and luminosity (44 ≲ log(
L
bol
/erg s
−1
) ≲ 48), and probe lower luminosities than an earlier compilation of SDSS DR7 quasars. Derived physical quantities such as single-epoch virial black hole masses and bolometric luminosities are also included in this catalog. We present improved systemic redshifts and realistic redshift uncertainties for DR16Q quasars using the measured line peaks and correcting for velocity shifts of various lines with respect to the systemic velocity. About 1%, 1.4%, and 11% of the original DR16Q redshifts deviate from the systemic redshifts by ∣Δ
V
∣ > 1500 km s
−1
, ∣Δ
V
∣ ∈ [1000, 1500] km s
−1
, and ∣Δ
V
∣ ∈ [500, 1000] km s
−1
, respectively; about 1900 DR16Q redshifts were catastrophically wrong (∣Δ
V
∣ > 10,000 km s
−1
). We demonstrate the utility of this data product in quantifying the spectral diversity and correlations among physical properties of quasars with large statistical samples.</description><subject>Astronomy & Astrophysics</subject><subject>Black holes</subject><subject>Luminosity</subject><subject>Physical properties</subject><subject>Quasars</subject><subject>Red shift</subject><subject>Sky surveys (astronomy)</subject><subject>Spectroscopy</subject><subject>Statistical analysis</subject><subject>Surveys</subject><subject>Velocity</subject><issn>0067-0049</issn><issn>1538-4365</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><recordid>eNp1kM1LwzAYh4MoOKd3j0HxZl2aJmlyHJtfMPBju4c0TWZn19SkFfbfm1HRi54CL8_vITwAnKfoJuMkn6Q04wnJGJ0oLYwqD8Do53QIRgixPEGIiGNwEsIGIZTTTIzAYgpnqlO1W0Nn4UuvgvLw2bvW-K4yAVrvtnBZO9XAebWuIgmX7zu47P2n2cF5nMJXUxsVDEzZKTiyqg7m7Psdg9Xd7Wr2kCye7h9n00WiCcq7xKa4KLWw1qJCUWKxsrhkiGgqeCFoQbhIaUGx5ZppKwguiOIlojgVmJQ0G4OLQetCV8mgq87oN-2axuhOYoIpYmmELgeo9e6jN6GTG9f7Jn5L4pxwQhlnLFJooLR3IXhjZeurrfI7mSK57yr3EeU-ohy6xsnVMKlc--tU7SaKWSaxJFi2pY3c9R_cv9ovcluFGg</recordid><startdate>20221201</startdate><enddate>20221201</enddate><creator>Wu, Qiaoya</creator><creator>Shen, Yue</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>OIOZB</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0003-1659-7035</orcidid><orcidid>https://orcid.org/0000-0003-4202-1232</orcidid><orcidid>https://orcid.org/0000000316597035</orcidid><orcidid>https://orcid.org/0000000342021232</orcidid></search><sort><creationdate>20221201</creationdate><title>A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16</title><author>Wu, Qiaoya ; Shen, Yue</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c407t-f12bdc9fff0ba54f2af2d604c598b95b48915b52f8c6cf942b4a8d0521924d53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Astronomy & Astrophysics</topic><topic>Black holes</topic><topic>Luminosity</topic><topic>Physical properties</topic><topic>Quasars</topic><topic>Red shift</topic><topic>Sky surveys (astronomy)</topic><topic>Spectroscopy</topic><topic>Statistical analysis</topic><topic>Surveys</topic><topic>Velocity</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wu, Qiaoya</creatorcontrib><creatorcontrib>Shen, Yue</creatorcontrib><creatorcontrib>US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)</creatorcontrib><collection>IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><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>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal. Supplement series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wu, Qiaoya</au><au>Shen, Yue</au><aucorp>US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16</atitle><jtitle>The Astrophysical journal. Supplement series</jtitle><stitle>APJS</stitle><addtitle>Astrophys. J. Suppl</addtitle><date>2022-12-01</date><risdate>2022</risdate><volume>263</volume><issue>2</issue><spage>42</spage><pages>42-</pages><issn>0067-0049</issn><eissn>1538-4365</eissn><abstract>We present a catalog of continuum and emission-line properties for 750,414 broad-line quasars included in the Sloan Digital Sky Survey Data Release 16 quasar catalog (DR16Q), measured from optical spectroscopy. These quasars cover broad ranges in redshift (0.1 ≲
z
≲ 6) and luminosity (44 ≲ log(
L
bol
/erg s
−1
) ≲ 48), and probe lower luminosities than an earlier compilation of SDSS DR7 quasars. Derived physical quantities such as single-epoch virial black hole masses and bolometric luminosities are also included in this catalog. We present improved systemic redshifts and realistic redshift uncertainties for DR16Q quasars using the measured line peaks and correcting for velocity shifts of various lines with respect to the systemic velocity. About 1%, 1.4%, and 11% of the original DR16Q redshifts deviate from the systemic redshifts by ∣Δ
V
∣ > 1500 km s
−1
, ∣Δ
V
∣ ∈ [1000, 1500] km s
−1
, and ∣Δ
V
∣ ∈ [500, 1000] km s
−1
, respectively; about 1900 DR16Q redshifts were catastrophically wrong (∣Δ
V
∣ > 10,000 km s
−1
). We demonstrate the utility of this data product in quantifying the spectral diversity and correlations among physical properties of quasars with large statistical samples.</abstract><cop>Saskatoon</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4365/ac9ead</doi><tpages>12</tpages><orcidid>https://orcid.org/0000-0003-1659-7035</orcidid><orcidid>https://orcid.org/0000-0003-4202-1232</orcidid><orcidid>https://orcid.org/0000000316597035</orcidid><orcidid>https://orcid.org/0000000342021232</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Astronomy & Astrophysics Black holes Luminosity Physical properties Quasars Red shift Sky surveys (astronomy) Spectroscopy Statistical analysis Surveys Velocity |
title | A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16 |
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