J/A+A/488/867ivo://CDS.VizieR/J/A+A/488/867doi:10.26093/cds/vizier.34880867CDSNieppola E.Valtaoja E.Tornikoski M.Hovatta T.Kotiranta M.2017-10-16T14:57:25Z2009-01-13T21:57:21ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiquasarsspectral-energy-distributionThe blazar sequence is a scenario in which the bolometric luminosity of the blazar governs the appearance of its spectral energy distribution. The most prominent result is the significant negative correlation between the synchrotron peak frequencies and the synchrotron peak luminosities of the blazar population. Observational studies of the blazar sequence have, in general, neglected the effect of Doppler boosting. We study the dependence of both the synchrotron peak frequency and luminosity with Doppler-corrected quantities. We determine the spectral energy distributions of 135 radio-bright AGN and find the best-fit parabolic function for the distribution to quantify their synchrotron emission. The corresponding measurements of synchrotron peak luminosities and frequencies are Doppler-corrected with a new set of Doppler factors calculated from variability data. The relevant correlations for the blazar sequence are determined for these intrinsic quantities.2008A&A...488..867Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/488/867CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/488/867https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/488/867http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/488/867https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/488/867https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/488/867http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/488/867GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/488/867/table1 (The sample and the observational synchrotron peak frequencies obtained in this work)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/488/867/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/488/867/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/488/867/table1?GETtext/xml+votable180.050000true1.5579167-6.393150.0055555555555555566/110 532 556 579 700 911 1263 1546 1576 1701 1782 2331 2397 2414 2836 3024 3096 3675 3820 3886 4027 4572 4695 4770 4820 5130 5139 5597 5693 5767 5806 5817 6252 6507 6641 6853 7226 7426 7570 7896 7969 8031 8057 8299 8487 8717 9442 9460 9612 9633 9723 10163 10249 10422 11430 11715 12301 12352 12580 12604 12619 12896 13352 13410 13496 13693 13927 14520 14737 14842 15067 15286 15494 15916 15936 16059 16093 16247 16281 16298 16301 17351 17579 17857 18035 18624 18661 19101 19190 19271 19370 19398 19567 19609 19831 20099 21358 21935 21968 21972 22274 22363 22396 22917 22950 23016 23099 23121 23127 23323 23416 24084 24123 24571 25864 26131 26292 26303 27060 27417 28083 28339 28479 28492 29570 29675 31190 31391 31430 31451 31664 31894 32764 40762 44908https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/488/867?format=asciiOpticaldefaultJ/A+A/488/867/table1The sample and the observational synchrotron peak frequencies obtained in this workrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource Name (HHMM+DDd or HHMM+DDMM)meta.id;meta.maincharONameOther namemeta.idcharClassAGN Classification (3)src.classcharlognup? Observational synchrotron peak frequency (1)log(Hz)em.freq;stat.maxfloatnullablen_lognup[1] Determination from highest flux density (2)meta.notecharz? Redshiftsrc.redshiftfloatnullableJy[*] * when in 1.2Jy AGN samplemeta.codecharBl[*] * when in Blazar samplemeta.codecharSimbadNameSimbad column added by the CDSmeta.idcharNEDSimbad column added by the CDScharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.main