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<ri:Resource created="2022-12-30T09:26:24Z" 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 and winds in BALQSOs</title><shortName>J/MNRAS/515/5159</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/515/5159</identifier><altIdentifier>doi:10.26093/cds/vizier.75155159</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Petley J.W.</name></creator><creator><name>Morabito L.K.</name></creator><creator><name>Alexander D.M.</name></creator><creator><name>Rankine A.L.</name></creator><creator><name>Fawcett V.A.,Rosario D.J.</name></creator><creator><name>Matthews J.H.</name></creator><creator><name>Shimwell T.M.</name></creator><creator><name>Drabent A.</name></creator><date role="Updated">2025-01-29T20:11:19Z</date><date role="Created">2022-12-30T09:26:24Z</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><description>Broad Absorption Line Quasars (BALQSOs) show strong signatures of powerful outflows, with the potential to alter the cosmic history of their host galaxies. These signatures are only seen in ~10% of optically selected quasars, although the fraction significantly increases in IR and radio selected samples. A proven physical explanation for this observed fraction has yet to be found, along with a determination of why this fraction increases at radio wavelengths. We present the largest sample of radio matched BALQSOs using the LOFAR Two-metre Sky Survey Data Release 2 and employ it to investigate radio properties of BALQSOs. Within the DR2 footprint, there are 3537 BALQSOs from Sloan Digital Sky Survey DR12 with continuum signal to noise &gt;=5. We find radio-detections for 1108 BALQSOs, with an important sub-population of 120 LoBALs, an unprecedented sample size for radio matched BALQSOs given the (sky) coverage to date. BALQSOs are a radio-quiet population that show an increase of x1.50 radio-detection fraction compared to non-BALQSOs. LoBALs show an increase of x2.22 that of non-BALQSO quasars. We show that this detection fraction correlates with wind-strength, reddening and CIV emission properties of BALQSOs and that these features may be connected, although no single property can fully explain the enhanced radio detection fraction. We create composite spectra for sub-classes of BALQSOs based on wind strength, colour, and radio properties, finding differences in the absorption profiles of radio-detected and radio-undetected sources, particularly for LoBALs. Overall, we favour a wind-ISM interaction explanation for the increased radio-detection fraction.</description><source format="bibcode">2022MNRAS.515.5159P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/515/5159</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/VIII/92">VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/279">VII/279 : SDSS quasar catalog: twelfth data release (Paris+, 2017)</relatedResource><relatedResource 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Quasar bolometric luminosity (Lbol)</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Lbol</name><description>? Quasar bolometric luminosity uncertainty (e_Lbol)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lognEdd</name><description>? log(Eddington fraction) (nEdd)</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RA2deg</name><description>? FIRST Right Ascension (J2000) (RAJ2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DE2deg</name><description>? FIRST Declination (J2000) (DEJ2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>F1.4peak</name><description>? FIRST 1.4GHz peak flux (Fpeak)</description><unit>mJy/beam</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F1.4int</name><description>? FIRST 1.4GHz integrated flux (Fint)</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>rms1.4</name><description>? FIRST 1.4GHz rms noise around source (Rms)</description><unit>mJy</unit><ucd>instr.det.noise</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Sep</name><description>? FIRST-LoTSS separation (Separation)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Bmagrest</name><description>? Estimated rest b-band luminosity (REST_B)</description><unit>W</unit><ucd>phys.luminosity;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logLRadio</name><description>? log(Rest frame 144MHz synchotron luminosity) (Radio_luminosity)</description><unit>log(W)</unit><ucd>phys.luminosity;em.radio</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>R</name><description>? 144MHz/B-band radio loudness (Radio_loudness)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>