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<ri:Resource created="2018-03-02T09:28:41Z" 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>Roma-BZCAT synchrotron peak &amp; Compton dominance</title><shortName>J/ApJ/841/113</shortName><identifier>ivo://CDS.VizieR/J/ApJ/841/113</identifier><altIdentifier>doi:10.26093/cds/vizier.18410113</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mao P.</name></creator><creator><name>Urry C.M.</name></creator><date role="Updated">2023-12-19T11:07:34Z</date><date role="Created">2018-03-02T09:28:41Z</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>bl-lacertae-objects</subject><subject>quasars</subject><description>We investigate a sample of 622 blazars with measured fluxes at 12 wavebands across the radio-to-gamma-ray spectrum but without spectroscopic or photometric redshifts. This sample includes hundreds of sources with newly analyzed X-ray spectra reported here. From the synchrotron peak frequencies, estimated by fitting the broadband spectral energy distributions (SEDs), we find that the fraction of high-synchrotron-peaked blazars in these 622 sources is roughly the same as in larger samples of blazars that do have redshifts. We characterize the no-redshift blazars using their infrared colors, which lie in the distinct locus called the WISE blazar strip, then estimate their redshifts using a KNN regression based on the redshifts of the closest blazars in the WISE color-color plot. Finally, using randomly drawn values from plausible redshift distributions, we simulate the SEDs of these blazars and compare them to known blazar SEDs. Based on all these considerations, we conclude that blazars without redshift estimates are unlikely to be high-luminosity, high- synchrotron-peaked objects, which had been suggested in order to explain the "blazar sequence"-an observed trend of SED shape with luminosity-as a selection effect. Instead, the observed properties of no-redshift blazars are compatible with a causal connection between jet power and electron cooling, i.e., a true blazar sequence.</description><source format="bibcode">2017ApJ...841..113M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/841/113</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/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/59">VIII/59 : the FIRST Survey, version 1999Jul (White+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/139">V/139 : The SDSS Photometric Catalog, DR9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalog, DR12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/323/757">J/MNRAS/323/757 : Deep X-Ray Radio Blazar Survey (DXRBS). II. (Landt+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/441">J/A+A/445/441 : SED of BL Lacertae objects (Nieppola+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/488/867">J/A+A/488/867 : Synchrotron peak frequency of 135 AGN (Nieppola+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/495/691">J/A+A/495/691 : Multifrequency catalog of blazars Roma-BZCAT (Massaro+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/68">J/ApJ/748/68 : WISE IR colors of gamma-ray blazars (D'Abrusco+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/26">J/ApJ/772/26 : AGN with WISE. II. The NDWFS Bootes field (Assef+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/12">J/ApJS/206/12 : Blazars with {gamma}-ray counterparts. I. (D'Abrusco+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/14">J/ApJS/215/14 : WISE {gamma}-ray blazar radio candidates (D'Abrusco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/23">J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/14">J/ApJ/810/14 : Third catalog of LAT-detected AGNs (3LAC) (Ackermann+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/26">J/ApJS/224/26 : SEDs of Roma BZCAT blazars (Mao+, 2016)</relatedResource><relatedResource>http://www.sdss3.org/ : SDSS-III home page</relatedResource><relatedResource>http://www.asdc.asi.it/bzcat/ : Roma BZCAT - 5th edition home page</relatedResource><relatedResource>http://fermi.gsfc.nasa.gov/ssc/data/access/lat/4yr_catalog/ : 3FGL home page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/841/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/841/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/841/113</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/841/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/841/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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44563 44592 44597 44604 44614 44624 44658 44661 44669-44670 44699 44705 44724 44730 44774 44776 44799 44805 44813 44818 44820 44832 44840 44899 44908 44944 45011 45016 45038 45081 45158-45159 45164-45165 45178 45196-45197 45286 45295 45303 45393 45409 45415 45424 45453 45482 45558 45575 45580 45599 45614 45621 45648 45655 45660 45690 45699 45713 45795 45803 45843 45846 45923 45943 45999 46055 46123 46142 46146 46175 46204 46214 46226 46232 46246 46251 46258 46310 46331 46337 46342 46354 46369-46370 46373-46374 46388 46404 46439 46445 46448 46459 46490 46521 46529 46542 46545-46546 46563 46568 46577 46588 46629 46717 46721 46724 46736 46740 46764 46787 46798 46810 46835 46844 46851-46852 46868 46872 46887 46918 46921 46932 46948 46951 46964-46966 46969 46994 47001 47014 47016 47050 47057 47080 47095 47106 47112 47151 47154 47248 47255 47319 47327 47341 47353-47354 47375 47413 47419 47512 47540 47564 47570 47605 47642 47649 47656 47672 47708 47714 47805 47847 47922 47941 47943 47969 47972 48023 48091 48108 48110 48120 48123 48137 48142 48187 48207 48238 48245 48284 48300 48306 48316 48320 48352 48362 48388 48407 48419 48422 48443 48460 48477 48483 48486 48496 48507 48582 48589 48595 48598 48610 48624 48629 48676 48685 48708 48716 48757 48767 48797-48798 48805 48814 48846 48878 48883 48893 48926 48965 48974-48975 48985 48989 48995 49019 49037 49069 49071 49084 49141</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/841/113?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/841/113/table3</name><description>*Synchrotron peak and Compton dominance for samples I and II</description><column><name>n_logPkC</name><description>Note on logPkC (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>logPkCr</name><description>[18/25]? Log rest frame Compton peak frequency (2)</description><unit>log(Hz)</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_logPkCr</name><description>Note on logPkCr (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>AC</name><description>[-1.5/2.1]? Compton Dominance in observed frame (f_peak,C_/f_peak,s_)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ACr</name><description>[-1.1/2.6]? Compton Dominance corrected to rest frame (L_peak,C_/L_peak,s_; only for Sample I)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PapI</name><description>Display data from Paper I (Mao+, 2016, J/ApJS/224/26) if any</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType><flag>nullable</flag></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>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></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>BZCAT</name><description>BZCAT identifier (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>logPk</name><description>[12/18]? Log observed frame synchrotron peak frequency (2)</description><unit>log(Hz)</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_logPk</name><description>Note on logPk (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>logPkr</name><description>[12/18]? Log rest frame synchrotron peak frequency (2)</description><unit>log(Hz)</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_logPkr</name><description>Note on logPkr (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="31*">char</dataType></column><column><name>logPkC</name><description>[19/25]? Log observed frame Compton peak frequency (2)</description><unit>log(Hz)</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>