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<ri:Resource created="2023-05-03T07:58:19Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Radio luminous QSOs in SDSS DR14Q</title><shortName>J/ApJ/922/202</shortName><identifier>ivo://CDS.VizieR/J/ApJ/922/202</identifier><altIdentifier>doi:10.26093/cds/vizier.19220202</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rusinek-Abarca K.</name></creator><creator><name>Sikora M.</name></creator><date role="Updated">2023-07-03T13:26:39Z</date><date role="Created">2023-05-03T07:58:19Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>quasars</subject><subject>active-galactic-nuclei</subject><subject>radio-sources</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>black-holes</subject><subject>galaxy-classification-systems</subject><description>While radio emission in quasars can be contributed to by a variety of processes (involving star-forming regions, accretion disk coronas and winds, and jets), the powering of the radio loudest quasars must involve very strong jets, presumably launched by the Blandford-Znajek mechanism incorporating the magnetically arrested disk (MAD) scenario. We focus on the latter and investigate the dependence of their fraction on redshift. We also examine the dependence of the radio-loud fraction (RLF) on BH mass (MBH) and Eddington ratio ({lambda}_Edd_), while excluding the redshift bias by narrowing its range. In both of these investigations, we remove the bias associated with: (1) the diversity of source selection by constructing two well-defined, homogeneous samples of quasars (first within 0.7&lt;=z&lt;=1.9, second within 0.5&lt;=zw=0.7); and (2) a strong drop in the RLF of quasars at smaller BH masses by choosing those with BH masses larger than 10^8.5^M_{sun}_. We confirm some of the previous results showing the increase in the fraction of radio-loud quasars with cosmic time and that this trend can be even steeper if we account for the bias introduced by the dependence of the RLF on BH mass, whereas the bias introduced by the dependence of the RLF on Eddington ratio is shown to be negligible. Assuming that quasar activities are triggered by galaxy mergers, we argue that such an increase can result from the slower drop with cosmic time of mixed mergers than of wet mergers.</description><source format="bibcode">2021ApJ...922..202R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/922/202</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/286">VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/289">VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/95/1">J/ApJS/95/1 : Atlas of Quasar Energy Distributions (Elvis+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/666">J/AJ/131/666 : Double-lobed radio quasars from the SDSS (de Vries+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/470">J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/658/815">J/ApJ/658/815 : Radio loudness of active galactic nuclei (Sikora+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/2302">J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A25">J/A+A/544/A25 : GPS radio sources multifrequency study (Mingaliev+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/62">J/ApJ/765/62 : SDSS-DR7 opt. sp. analysis of radio galaxies (Sikora+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/769/79">J/ApJ/769/79 : Spitzer obs. of radio-loud AGNs (CARLA) (Wylezalek+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/462/1910">J/MNRAS/462/1910 : H-ATLAS NGP LOFAR radio catalogue (Hardcastle+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/228/9">J/ApJS/228/9 : Physical param. of ~300000 SDSS-DR12 QSOs (Kozlowski, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/233/17">J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. 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27052 27059 27067 27069-27070 27073-27076 27078 27093-27095 27101 27108 27110-27111 27114 27117-27118 27120 27125-27127 27133 27199 27220 27222 27226 27229 27234-27235 27238 27243 27246 27250-27251 27257 27259 27287-27288 27303 27308-27309 27313 27318-27320 27325-27329 27332 27336-27338 27342 27348-27349 27351-27353 27355-27356 27364 27367 27376 27379 27381 27388 27391 27399 27404 27407 27409 27416 27428-27430 27433 27437 27444-27445 27447 27449 27453 27455-27457 27462 27464 27466 27471 27478-27480 27482 27484 27492-27493 27504-27506 27510-27511 27516 27519 27527 27541-27542 27544 27554 27557-27558 27560 27564 27570-27571 27580 27583 27587 27593 27596-27597 27602 27605 27611 27615 27617 27619 27622-27623 27628 27630 27633-27635 27644 27651-27652 27658 27666 27671 27674-27675 27680-27682 27687-27688 27691 27699 27717-27722 27725 27727 27734 27737-27739 27741-27742 27745 27748 27763 27765 27778-27779 27782 27785-27786 27789 27795-27796 27800 27803 27805-27806 27810 27813 27815 27818 27821 27825-27826 27836 27841 27844 27846 27848-27849 27860 27862 27865 27868 27872 27875-27876 27879 27883-27884 27890 27893-27895 27897-27898 27901-27902 27910-27911 27913 27917 27922 27925-27926 27931 27935 27939-27940 27943 27950 27952 27954-27955 27957 27963 27966 27970-27971 27976 27982-27983 27986 27990 27993 27995 27997 27999 28005-28006 28010-28011 28013 28022 28037-28040 28059 28062 28064-28065 28070-28071 28078 28081 28085 28087-28089 28096 28104 28110 28116-28117 28121 28125 28128 28130-28134 28141-28143 28149 28154 28156 28158 28161 28167-28168 28176 28179-28180 28183-28184 28187 28189 28192 28196 28199-28202 28205 28208-28210 28216 28233-28234 28239 28242 28246-28247 28249 28256 28260 28266 28269 28274-28275 28278 28289 28292 28295 28297-28298 28311-28312 28314 28317 28321 28323 28330-28331 28333 28340-28341 28345 28354 28359 28361-28363 28365 28367 28369 28373 28375 28382 28386 28395-28396 28400-28401 28412 28419 28426 28432 28438-28439 28441 28445-28446 28448 28457 28470 28473 28476-28477 28486-28487 28491 28493-28494 28497 28502 28504 28507-28509 28513 28519 28521-28523 28526 28531-28533 28536-28538 28540-28541 28545 28548 28553 28555 28561-28562 28564 28566 28569 28574 28580-28581 28586-28587 28589 28594-28598 28603 28611 28616 28620-28621 28627 28632-28633 28636 28644 28648 28654 28658 28660-28661 28667 28669 28671 31292-31293 31332 31344-31345 31357 31374 31381-31382 31384-31385 31391 31402-31404 31408 31414 31420 31430 31434-31438 31441 31443 31448 31450 31453-31454 31456 31459 31464 31466 31472-31473 31477 31479 31482-31484 31531 31550 31594 31612 31616 31618 31624-31625 31627 31631 31636 31639-31640 31642 31648 31651 31658-31661 31663 31667-31668 31672 31674 31677 31679 31684 31689 31693 31696-31697 31715 31720-31721 31728-31729 31731-31732 31737 31739 31741-31742 32406 32411 32414-32415 32421 32427 32429-32430 32435 32438-32439 32444-32446 32457 32481 32483 32489 32491 32494 32511 36763 36767 36775-36776 36781 36786-36787 36802-36803 45046-45047 45052-45054 49009 49013-49014 49016 49091 49101-49102 49106</spatial><spectral>9.276497240453405e-25 9.276497240453405e-25</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/922/202?format=ascii</footprint><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/922/202/tableb1</name><description>0.5-0.7 QSOs (total of 3511 objects) used in this study</description><column><name>LEDA</name><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SDSS</name><description>SDSS identifier (HHMMSS.ss+DDMMSS.s; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>z</name><description>[0.5/0.7] Spectroscopic redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMBH</name><description>[8.5/10.3] log Black Hole mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLb</name><description>[44/47.1] log bolometric luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logEdd</name><description>[-3.3/-0.07] log Eddington ratio</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F1.4</name><description>[0.6/6626] The 1.4GHz flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ratio</name><description>[0.49/56027] The 1.4GHz/i band luminosity ratio</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Class</name><description>Radio class (1)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Morph</name><description>Radio morphology (2)</description><ucd>meta.code;src.morph</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>G19</name><description>Display data from Guerkan+, 2019, J/A+A/622/A11</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Sloan</name><description>Display the online SDSS-DR16 data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>NED column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from SDSS names (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from SDSS names (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>