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<ri:Resource created="2013-11-28T09:01:22Z" 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>AMIGA. Revision of the isolation degree</title><shortName>J/A+A/560/A9</shortName><identifier>ivo://CDS.VizieR/J/A+A/560/A9</identifier><altIdentifier>doi:10.26093/cds/vizier.35600009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Argudo-Fernandez M.</name></creator><creator><name>Verley S.</name></creator><creator><name>Bergond G.</name></creator><creator><name>Sulentic J.</name></creator><creator><name>Sabater J.,Fernandez Lorenzo M.</name></creator><creator><name>Leon S.</name></creator><creator><name>Espada D.</name></creator><creator><name>Verdes-Montenegro L.,Santander-Vela J.D.</name></creator><creator><name>Ruiz J.E.</name></creator><creator><name>Sanchez-Exposito S.</name></creator><date role="Updated">2017-10-09T13:33:58Z</date><date role="Created">2013-11-28T09:01:22Z</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>photometry</subject><subject>spectroscopy</subject><description>To understand the evolution of galaxies, it is necessary to have a reference sample where the effect of the environment is minimized and quantified. In the framework of the AMIGA project (Analysis of the interstellar Medium of Isolated GAlaxies), we present a revision of the environment for galaxies in the Catalogue of Isolated Galaxies (CIG, Karachentseva 1973, Cat. VII/82) using the ninth data release of the Sloan Digital Sky Survey (SDSS-DR9). The aims of this study are to refine the photometric-based AMIGA sample of isolated galaxies and to provide an improvement of the quantification of the isolation degree with respect to previous works, using both photometry and spectroscopy. We developed an automatic method to search for neighbours within a projected area of 1Mpc radius centred on each primary galaxy to revise the CIG isolation criteria introduced by Karachentseva (1973, Cat. VII/82). The local number density at the fifth nearest neighbour and the tidal strength affecting the CIG galaxy were estimated to quantify the isolation degree. Of the 636 CIG galaxies considered in the photometric study, 426 galaxies fulfil the CIG isolation criteria within 1Mpc, taking into account projected neighbours. Of the 411 CIG galaxies considered in the spectroscopic study, 347 galaxies fulfil the CIG isolation criteria when a criterion about redshift difference is added. The available redshifts allow us to reject background neighbours and thus improve the photometric assessment. On average, galaxies in the AMIGA sample show lower values in the local number density and the tidal strength parameters than galaxies in denser environments such as pairs, triplets, compact groups, and clusters. For the first time, the environment and the isolation degree of AMIGA galaxies are quantified using digital data. The use of the SDSS database permits one to identify fainter and smaller-size satellites than in previous AMIGA works. The AMIGA sample is improved by this study, because we reduced the sample of isolated galaxies used in previous AMIGA works by about 20%. The availability of the spectroscopic data allows us to check the validity of the CIG isolation criteria, which is not fully efficient. About 50% of the neighbours considered as potential companions in the photometric study are in fact background objects. We also find that about 92% of the neighbour galaxies that show recession velocities similar to the corresponding CIG galaxy are not considered by the CIG isolation criteria as potential companions, which may have a considerable influence on the evolution of the central CIG galaxy.</description><source format="bibcode">2013A&amp;A...560A...9A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/560/A9</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/VII/82">VII/82 : Catalogue of Isolated Galaxies (Karachentseva+ 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/411/391">J/A+A/411/391 : AMIGA project Revised positions for CIG galaxies (Leon+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/436/443">J/A+A/436/443 : AMIGA I. Velocities of CIG galaxies (Verdes-Montenegro+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/449/937">J/A+A/449/937 : AMIGA II. Morphological refinement (Sulentic+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/462/507">J/A+A/462/507 : AMIGA III. IRAS data (Lisenfeld+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/470/505">J/A+A/470/505 : AMIGA IV. Neighbours around CIG galaxies (Verley+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/472/121">J/A+A/472/121 : AMIGA V. Isolation parameters (Verley+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/485/475">J/A+A/485/475 : AMIGA VI. Radio fluxes of the isolated galaxies (Leon+ 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/73">J/A+A/486/73 : AMIGA VII. FIR and radio study (Sabater+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/532/A117">J/A+A/532/A117 : AMIGA VIII. Flux ratio asymmetry parameter (Espada+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A102">J/A+A/534/A102 : AMIGA IX. Molecular gas properties (Lisenfeld+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A47">J/A+A/540/A47 : AMIGA X. Isolated galaxy colors (Fernandez Lorenzo+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/545/A15">J/A+A/545/A15 : AMIGA XI. Optical nuclear activity (Sabater+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/1756">J/MNRAS/397/1756 : Fourier-derived parameters of CIG sample (Durbala+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/434/325">J/MNRAS/434/325 : 452 AMIGA galaxies physical param. 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