J/MNRAS/427/1135ivo://CDS.VizieR/J/MNRAS/427/1135doi:10.26093/cds/vizier.74271135CDSDiPompeo M.A.Brotherton M.S.Cales S.L.Runnoe J.C.2024-07-19T20:16:59Z2013-10-11T09:11:46ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frquasarsultraviolet-astronomyline-intensitiesWe recently presented radio observations of a large sample of radio-loud broad absorption line (BAL) quasars from the Sloan Digital Sky Survey (SDSS) and Faint Images of the Radio Sky at Twenty-cm surveys, as well as a well matched sample of unabsorbed quasars, primarily to measure their radio spectral indices and estimate ensemble orientations. Here, we analyse the SDSS spectra of these samples and compare the rest-frame ultraviolet properties of radio-loud BAL and non-BAL quasars. Ultraviolet properties include the continuum shape, emission-line measurements of CIV, AlIII, CIII], FeII and MgII, and BAL properties including the balnicity index, absorption index and minimum and maximum outflow velocities. We find that radio-loud BAL quasars have similar ultraviolet properties compared to radio-loud non-BAL sources, though they do appear to have redder continua and stronger FeII emission, which is consistent with what is found for radio-quiet BAL sources. No correlations exist between outflow properties and orientation (radio spectral index), suggesting that BAL winds along any line of sight are driven by the same mechanisms. There are also few correlations between spectral index and other properties. We conclude that BAL outflows occur along all lines of sight with similar strengths and velocities.2012MNRAS.427.1135Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/427/1135CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/427/107 : Polarization in BAL QSOs (Lamy+, 2004)J/ApJS/165/1 : BAL QSOs from SDSS DR3 (Trump+, 2006)J/ApJ/665/990 : SDSS DR2 BAL QSOs (Ganguly+, 2007)J/ApJ/692/758 : BAL QSOs in SDSS-DR5 (Gibson+, 2009)J/MNRAS/410/860 : Redshift dependence of BAL QSOs (Allen+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/427/1135https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/427/1135http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/427/1135https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/427/1135https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/427/1135http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/427/1135GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/427/1135/BALs (Properties and line measurements of the sample of radio-loud BAL quasars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/427/1135/BALs?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/427/1135/BALs?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/427/1135/BALs?GETtext/xml+votable180.050000true3.53425-8.87838890.0055555555555555566/4103 4164 4228 4234 4362 4787 4959 4976 5008 5047 5055 5072 5087 5103 5109 5236 5302 5332 5336 5342-5343 5364 5429 5441 5452 5477 5485-5486 5638 5648 5651 5666 5704 5706 5732 5764 5766 5771 5942 6098 6227 6230 6236 6248 6357 6403 6421 6464 6470-6471 6487 6642 6644 7256 7316 7568 9164-9165 9172 9365 9381 9385 9452 9464 9466 9515 9613-9614 9729 9778 9788 9826 9859 9877 9890 9896 9929 10027 10318 10351 10356 10429 10433 10481 10486 10509 10535 10538 10551 10592 10634 10642 10688 10736 10802 10808 10814 10827 10829 10902 10912 10968 11249 11264-11265 11389 11398 11408 11436 17215 17261 17522 17758 18068 18086 18090 18097 18112 25844 25947 26212 26222 26239 26258 26285 26558 27021 27048 27420 27487 27501 27576 27595 27650 27699 27728 28204 28538 28587 28640 28671 31396 32486https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/427/1135?format=asciiUVdefaultJ/MNRAS/427/1135/BALsProperties and line measurements of the sample of radio-loud BAL quasarszRedshiftsrc.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNote[n] n for non-BAL samplemeta.notecharSDSSSDSS name (JHHMMSS.ss+DDMMSS.s)meta.id;meta.maincharlogR*[0.98/3.25] Radio loudnessphot.flux;arith.ratiofloatlogLrRadio luminosity, k-corrected to rest-frame 5GHzlog(1e-07W)phys.luminosity;em.radio.3-6GHzfloatlogLbolBolometric luminositylog(1e-07W)phys.luminosityfloatlogMbh? Black-hole masslog(solMass)phys.massfloatnullablefEdd[0/3.1]? Eddington fraction (Lbol/Ledd)phys.luminosity;arith.ratiofloatnullablel_BILimit flag on BImeta.code.errorcharBI? Balnicity index (1)km/smeta.code;spect.indexintnullablel_AILimit flag on AImeta.code.errorcharAI? Absorption index (1) (2)km/sspect.indexintnullablel_vmaxLimit on vmaxmeta.code.errorcharvmax? Maximum velocity (1)km/sphys.velocintnullablevmin? Minimum velocity (1)km/sphys.velocintnullableSloanDisplay the SDSS data for this quasarmeta.ref.urlcharObjectObject short name (HHMM+DDMM)meta.idcharf1000Continuum normalized flux density at 1000km/s, in 10^-17^erg/cm^2^/s/{AA} (1)1e-19W.m**-2.nm**-1phot.fluxfloatalphaUVPower-law slope {alpha}_UV_, F_{lambda}_{prop.to}{lambda}^-{alpha}^ (1)spect.indexfloatFeIIFeII scaling factor (1) (2)arith.factorfloatEW(CIV)? CIV equivalent width0.1nmspect.line.eqWidthfloatnullablee_EW(CIV)? rms uncertainty on EW(CIV)0.1nmstat.errorfloatnullableFW(CIV)? CIV FWHMkm/sspect.line.widthintnullablee_FW(CIV)? rms uncertainty on FW(IV)km/sstat.errorintnullableBS(CIV)? CIV blueshiftkm/sspect.dopplerVelocfloatnullableEW(AlIII)? AlIII equivalent width (3)0.1nmspect.line.eqWidthfloatnullablee_EW(AlIII)? rms uncertainty on EW(AlIII)0.1nmstat.errorfloatnullableFW(AlIII)? AlIII FWHMkm/sspect.line.widthintnullablee_FW(AlIII)? rms uncertainty on FW(AlIII)km/sstat.errorintnullableEW[CIII]? [CIII] equivalent width (3)0.1nmspect.line.eqWidthfloatnullablee_EW[CIII]? rms uncertainty on EW[CIII]0.1nmstat.error;spect.line.eqWidthfloatnullableFW[CIII]? [CIII] FWHMkm/sspect.line.widthintnullablee_FW[CIII]? rms uncertainty on FW[CIII]km/sstat.errorintnullableBS[CIII]? [CIII] blueshiftkm/sspect.dopplerVelocfloatnullableEW(MgII)? MgII equivalent width0.1nmspect.line.eqWidthfloatnullablee_EW(MgII)? rms uncertainty on EWMgII0.1nmstat.errorfloatnullableFW(MgII)? MgII FWHMkm/sspect.line.widthintnullablee_FW(MgII)? rms uncertainty on FW(MgII)km/sstat.errorintnullableBS(MgII)? MgII blueshiftkm/sspect.dopplerVelocfloatnullable_RARight ascension (derived from SDSS) for Eq=J2000degpos.eq.ra;meta.main_DEDeclination (derived from SDSS) for Eq=J2000degpos.eq.dec;meta.main