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<ri:Resource created="2017-04-04T13:38:09Z" 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>Classical Cepheids in MCs. I. LMC disk</title><shortName>J/ApJ/832/176</shortName><identifier>ivo://CDS.VizieR/J/ApJ/832/176</identifier><altIdentifier>doi:10.26093/cds/vizier.18320176</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Inno L.</name></creator><creator><name>Bono G.</name></creator><creator><name>Matsunaga N.</name></creator><creator><name>Fiorentino G.</name></creator><creator><name>Marconi M.</name></creator><creator><name>Lemasle B.,da Silva R.</name></creator><creator><name>Soszynski I.</name></creator><creator><name>Udalski A.</name></creator><creator><name>Romaniello M.</name></creator><creator><name>Rix H.-W.</name></creator><date role="Updated">2018-12-04T10:42:41Z</date><date role="Created">2017-04-04T13:38:09Z</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>magellanic-clouds</subject><subject>variable-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>interstellar-reddening</subject><subject>stellar-distance</subject><description>We present a detailed investigation of the Large Magellanic Cloud (LMC) disk using classical Cepheids. Our analysis is based on optical (I, V; OGLE-IV), near-infrared (NIR: J, H, K_S_) and mid-infrared (MIR: w1; WISE) mean magnitudes. By adopting new templates to estimate the NIR mean magnitudes from single-epoch measurements, we build the currently most accurate, largest, and homogeneous multi-band data set of LMC Cepheids. We determine Cepheid individual distances using optical and NIR Period-Wesenheit relations (PWRs), to measure the geometry of the LMC disk and its viewing angles. Cepheid distances based on optical PWRs are precise at 3%, but accurate to 7%, while the ones based on NIR PWRs are more accurate (to 3%), but less precise (2%-15%), given the higher photometric error on the observed magnitudes. We found an inclination of i=25.05+/-0.02(stat.)+/-0.55(syst.){deg}, and a position angle of the lines of nodes P.A.=150.76+/-0.02(stat.)+/-0.07(syst.){deg}. These values agree well with estimates based either on young (Red Supergiants) or on intermediate-age (Asymptotic Giant Branch, Red Clump) stellar tracers, but they significantly differ from evaluations based on old (RR Lyrae) stellar tracers. This indicates that young/intermediate and old stellar populations have different spatial distributions. Finally, by using the reddening-law fitting approach, we provide a reddening map of the LMC disk, which is 10 times more accurate and 2 times larger than similar maps in the literature. We also found an LMC true distance modulus of {mu}_0,LMC_=18.48+/-0.10(stat. and syst.)mag, in excellent agreement with the currently most accurate measurement.</description><source format="bibcode">2016ApJ...832..176I</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/832/176</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/221">I/221 : The Magellanic Catalogue of Stars - MACS (Tucholke+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/305">II/305 : SAGE LMC and SMC IRAC Source Catalog (IPAC 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/288">II/288 : IRSF Magellanic Clouds Point Source Catalog (Kato+ 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/33">IV/33 : Master Catalogue towards the Magellanic Clouds (MC2) (Delmotte+ 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/228">II/228 : DENIS Catalogue toward Magellanic Clouds (DCMC) (Cioni+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/580/A18">J/A+A/580/A18 : Carina Project VIII. {alpha}-element abund. 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