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<ri:Resource created="2019-12-27T13:14:59Z" 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>Far-infrared SED measurements of massive galaxies</title><shortName>J/ApJ/869/4</shortName><identifier>ivo://CDS.VizieR/J/ApJ/869/4</identifier><altIdentifier>doi:10.26093/cds/vizier.18690004</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>De Rossi M.E.</name></creator><creator><name>Rieke G.H.</name></creator><creator><name>Shivaei I.</name></creator><creator><name>Bromm V.</name></creator><creator><name>Lyu J.</name></creator><date role="Updated">2020-04-17T08:24:56Z</date><date role="Created">2019-12-27T13:14:59Z</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>infrared-sources</subject><subject>redshifted</subject><subject>astronomical-reference-materials</subject><subject>spectral-energy-distribution</subject><description>Massive Population II galaxies undergoing the first phase of vigorous star formation after the initial Population III stage should have high energy densities and silicate-rich interstellar dust. We have modeled the resulting far-infrared spectral energy distributions (SEDs), demonstrating that they are shifted substantially to bluer ("warmer") wavelengths relative to the best fitting ones at z~3, and with strong outputs in the 10-40{mu}m range. When combined with a low level of emission by carbon dust, their SEDs match that of Haro 11, a local moderately low-metallicity galaxy undergoing a very young and vigorous starburst that is likely to approximate the relevant conditions in young Population II galaxies. We expect to see similar SEDs at high redshifts (z&gt;~5) given the youth of galaxies at this epoch. In fact, we find a progression with redshift in observed galaxy SEDs, from those resembling local ones at 2&lt;~z&lt;4 to a closer resemblance with Haro 11 at 5&lt;~z&lt;7. In addition to the insight on conditions in high-redshift galaxies, this result implies that estimates of the total infrared luminosities at z~6 based on measurements near {lambda}~1mm can vary by factors of 2-4, depending on the SED template used. Currently popular modified blackbodies or local templates can result in significant underestimates compared with the preferred template based on the SED of Haro 11.</description><source format="bibcode">2018ApJ...869....4D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/869/4</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/ApJS/95/1">J/ApJS/95/1 : Atlas of Quasar Energy Distributions (Elvis+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/684/136">J/ApJ/684/136 : SEDs of ELAIS-S1 mid-IR sources (Gruppioni+, 2008)</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/738/69">J/ApJ/738/69 : SEDs of galaxies at 3.8&lt;z&lt;5 in GOODS (Shim+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A119">J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A109">J/A+A/527/A109 : Dust and PAH emission SEDs of disk galaxies (Popescu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A100">J/A+A/551/A100 : Panchromatic SED of Herschel sources (Berta+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A66">J/A+A/557/A66 : Effective SEDs of IR gal. at various z (Bethermin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/565/A128">J/A+A/565/A128 : Dust SED in HRS nearby galaxies (Ciesla+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/582/A121">J/A+A/582/A121 : Dust properties in galaxies (Remy-Ruyer+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/219/18">J/ApJS/219/18 : LIRAS: LoCuSS IR AGN survey (Xu+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/462/1989">J/MNRAS/462/1989 : HerMES Large Mode Survey catalogue (Asboth+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/822/109">J/ApJ/822/109 : MIR view of polar dust emission in local AGNs (Asmus+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/229/25">J/ApJS/229/25 : GOALS sample PACS and SPIRE fluxes (Chu+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/841/76">J/ApJ/841/76 : Intrinsic far-IR SED of luminous AGNs (Lyu+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/609/A130">J/A+A/609/A130 : [CII] luminosities of gal. in G.A.S.+Cloudy (Lagache+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/609/A30">J/A+A/609/A30 : Conversion factors to LIR &amp; 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