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<ri:Resource created="2016-01-06T15:15:07Z" status="active" updated="2025-06-13T15:25:00Z" 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>VMC survey. XIV. SFR in SMC</title><shortName>J/MNRAS/449/639</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/449/639</identifier><altIdentifier>doi:10.26093/cds/vizier.74490639</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rubele S.</name></creator><creator><name>Girardi L.</name></creator><creator><name>Kerber L.</name></creator><creator><name>Cioni M.-R.L.</name></creator><creator><name>Piatti A.E.</name></creator><creator><name>Zaggia S.,Bekki K.</name></creator><creator><name>Bressan A.</name></creator><creator><name>Clementini G.</name></creator><creator><name>De Grijs R.</name></creator><creator><name>Emerson J.P.,Groenewegen M.A.T.</name></creator><creator><name>Ivanov V.D.</name></creator><creator><name>Marconi M.</name></creator><creator><name>Marigo P.</name></creator><creator><name>Moretti M.-I.,Ripepi V.</name></creator><creator><name>Subramanian S.</name></creator><creator><name>Tatton B.L.</name></creator><creator><name>Van Loon J.T.</name></creator><date role="Updated">2024-08-14T20:21:29Z</date><date role="Created">2016-01-06T15:15:07Z</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>stellar-distance</subject><subject>extinction</subject><description>We analyse deep images from the VISTA survey of the Magellanic Clouds in the YJKs filters, covering 14deg^2^ (10 tiles), split into 120 subregions, and comprising the main body and Wing of the Small Magellanic Cloud (SMC). We apply a colour-magnitude diagram reconstruction method that returns their best-fitting star formation rate SFR(t), age-metallicity relation (AMR), distance and mean reddening, together with 68 percent confidence intervals. The distance data can be approximated by a plane tilted in the East-West direction with a mean inclination of 39{deg}, although deviations of up to +/-3kpc suggest a distorted and warped disc. After assigning to every observed star a probability of belonging to a given age-metallicity interval, we build high-resolution population maps. These dramatically reveal the flocculent nature of the young star-forming regions and the nearly smooth features traced by older stellar generations. They document the formation of the SMC Wing at ages &lt;0.2Gyr and the peak of star formation in the SMC Bar at ~40Myr. We clearly detect periods of enhanced star formation at 1.5 and 5Gyr. The former is possibly related to a new feature found in the AMR, which suggests ingestion of metal-poor gas at ages slightly larger than 1Gyr. The latter constitutes a major period of stellar mass formation. We confirm that the SFR(t) was moderately low at even older ages.</description><source format="bibcode">2015MNRAS.449..639R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/449/639</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/MNRAS/424/1807">J/MNRAS/424/1807 : VISTA Magellanic Cloud Survey. V. Cepheids (Ripepi+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A29">J/A+A/549/A29 : Quasars behind the Magellanic system (Cioni+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/554/A33">J/A+A/554/A33 : VMC Survey. 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