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<ri:Resource created="2021-04-19T10:35:26Z" 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>PAH features of star-forming gal. using Spitzer/IRS</title><shortName>J/ApJ/884/136</shortName><identifier>ivo://CDS.VizieR/J/ApJ/884/136</identifier><altIdentifier>doi:10.26093/cds/vizier.18840136</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Xie Y.</name></creator><creator><name>Ho L.C.</name></creator><date role="Updated">2021-07-05T11:16:30Z</date><date role="Created">2021-04-19T10:35:26Z</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>galaxies</subject><subject>spectroscopy</subject><subject>infrared-sources</subject><subject>redshifted</subject><subject>stellar-masses</subject><subject>chemical-abundances</subject><subject>extinction</subject><description>Polycyclic aromatic hydrocarbon (PAH) emission has long been proposed to be a potential star formation rate indicator, as it arises from the photodissociation region bordering the Stromgren sphere of young, massive stars. We apply a recently developed technique of mid-infrared spectral decomposition to obtain a uniform set of PAH measurements from Spitzer low-resolution spectra of a large sample of star-forming galaxies spanning a wide range in stellar mass (M_*_~10^6^-10^11.4^M_{sun}_) and star formation rate (~0.1-2000M_{sun}_/yr). High-resolution spectra are also analyzed to measure [NeII]12.8{mu}m and [NeIII]15.6{mu}m, which effectively trace the Lyman continuum. We present a new relation between PAH luminosity and star formation rate based on the [NeII] and [NeIII] lines. Calibrations are given for the integrated 5-15{mu}m PAH emission, the individual features at 6.2, 7.7, 8.6, and 11.3{mu}m, as well as several mid- infrared bandpasses sensitive to PAH. We confirm that PAH emission is suppressed in low-mass dwarf galaxies, and we discuss the possible physical origin of this effect.</description><source format="bibcode">2019ApJ...884..136X</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/884/136</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/J/ApJ/511/639">J/ApJ/511/639 : Abundances in blue compact galaxies (Izotov+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/522/113">J/ApJ/522/113 : 1Jy IRAS galaxies optical spectroscopy (Veilleux+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/648/987">J/ApJ/648/987 : UV through far-IR analysis of M81 (Perez-Gonzalez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/671/323">J/ApJ/671/323 : Spitzer Spectra of a 10mJy galaxy sample (Houck+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/656/770">J/ApJ/656/770 : Mid-IR spectrum of star-forming galaxies (Smith+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/127">J/ApJ/686/127 : Starbursts luminosities based on PAH (Weedman+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/517">J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/1672">J/ApJ/703/1672 : Far-IR and H{alpha} fluxes in galaxies (Kennicutt+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/885">J/ApJ/705/885 : PAH in galaxies at z~0.1 (O'Dowd+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/556">J/ApJ/692/556 : Star forming galaxy templates (Rieke+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/1398">J/ApJ/701/1398 : SFR for starburst galaxies (Sargsyan+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/714/1256">J/ApJ/714/1256 : Far-IR star formation rate indicators (Calzetti+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/719/1191">J/ApJ/719/1191 : Mid-IR indicators of SF and AGN in galaxies (Treyer+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/79">J/ApJ/741/79 : The Spitzer-SDSS-GALEX Spectroscopic Survey (O'Dowd+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/819/L27">J/ApJ/819/L27 : Stellar masses of optical &amp; 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