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<ri:Resource created="2022-06-13T08:22:52Z" 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>Iron template spectrum from Mrk493 HST/STIS obs.</title><shortName>J/ApJS/258/38</shortName><identifier>ivo://CDS.VizieR/J/ApJS/258/38</identifier><altIdentifier>doi:10.26093/cds/vizier.22580038</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Park D.</name></creator><creator><name>Barth A.J.</name></creator><creator><name>Ho L.C.</name></creator><creator><name>Laor A.</name></creator><date role="Updated">2022-09-07T13:28:54Z</date><date role="Created">2022-06-13T08:22:52Z</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>seyfert-galaxies</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>quasars</subject><subject>redshifted</subject><description>We present a new empirical template for iron emission in active galactic nuclei (AGNs) covering the 4000-5600{AA} range. The new template is based on a spectrum of the narrow-line Seyfert 1 galaxy Mrk 493 obtained with the Hubble Space Telescope. In comparison with the canonical iron template object I Zw 1, Mrk 493 has narrower broad-line widths, lower reddening, and a less extreme Eddington ratio, making it a superior choice for template construction. We carried out a multicomponent spectral decomposition to produce a template incorporating all the permitted and forbidden lines of FeII identified in the Mrk 493 spectrum over this wavelength range, as well as lines from TiII, NiII, and CrII. We tested the template by fitting it to AGN spectra spanning a broad range of iron emission properties, and we present a detailed comparison with fits using other widely used monolithic and multicomponent iron emission templates. The new template generally provides the best fit (lowest {chi}2) compared to other widely used monolithic empirical templates. In addition, the new template yields more accurate spectral measurements including a significantly better match of the derived Balmer line profiles (H{beta}, H{gamma}, H{delta}), in contrast with results obtained using the other templates. Our comparison tests show that the choice of iron template can introduce a systematic bias in measurements of the H{beta} line width, which consequently impacts single-epoch black hole mass estimates by ~0.1dex on average and possibly up to ~0.3-0.5dex individually.</description><source format="bibcode">2022ApJS..258...38P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/258/38</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/I/294">I/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</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/145/199">J/ApJS/145/199 : Optical spectroscopic atlas of low-z AGN (Marziani+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/152/251">J/ApJS/152/251 : Indo-US library of coude feed stellar spectra (Valdes+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/417/515">J/A+A/417/515 : I Zw 1 unusual emission line spectrum (Veron-Cetty+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/670/92">J/ApJ/670/92 : New sample of low-mass black holes in AGN (Greene+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/581">J/MNRAS/383/581 : Broad-line Balmer decrements in blue AGN (Dong+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/78">J/ApJ/687/78 : FeII emission in quasars (Hu+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/680/169">J/ApJ/680/169 : SDSS DR5 virial black hole masses (Shen+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/674/668">J/ApJ/674/668 : SDSS J102839.11+450009.4 Fe II emission lines (Wang+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/189/15">J/ApJS/189/15 : FeII emission in a sample of AGN spectra (Kovacevic+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/86">J/ApJ/736/86 : FeII emission in SDSS type 1 AGNs (Dong+, 2011)</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/ApJ/746/169">J/ApJ/746/169 : Luminosity function of broad-line quasars (Shen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/125">J/ApJ/753/125 : NIR spectroscopy follow-up of 60 SDSS-DR7 QSOs (Shen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/45">J/ApJ/764/45 : Luminosity function of broad-line quasars. 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