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<ri:Resource created="2000-04-28T11:38:09Z" 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>Spiral and lenticular galaxy brightness profiles</title><shortName>J/AJ/116/1626</shortName><identifier>ivo://CDS.VizieR/J/AJ/116/1626</identifier><altIdentifier>doi:10.26093/cds/vizier.51161626</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Baggett W.E.</name></creator><creator><name>Baggett S.M.</name></creator><creator><name>Anderson K.S.J.</name></creator><date role="Updated">2023-04-06T16:50:29Z</date><date role="Created">2000-04-28T11:38:09Z</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>galaxies</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>galaxy-classification-systems</subject><description>We present one of the largest homogeneous sets of spiral and lenticular galaxy brightness profile decompositions completed to date. The 659 galaxies in our sample have been fitted with a de Vaucouleurs law for the bulge component and an inner-truncated exponential for the disk component. Of the 659 galaxies in the sample, 620 were successfully fitted with the chosen fitting functions. The fits are generally well defined, with more than 90% having rms deviations from the observed profile of less than 0.35mag. We find no correlations of fitting quality, as measured by these rms residuals, with either morphological type or inclination. Similarly, the estimated errors of the fitted coefficients show no significant trends with type or inclination. These decompositions form a useful basis for the study of the light distributions of spiral and lenticular galaxies. The object base is sufficiently large that well-defined samples of galaxies can be selected from it.</description><source format="bibcode">1998AJ....116.1626B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/116/1626</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/118">VII/118 : NGC 2000.0 (Sky Publishing, ed. 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Minimum value of second fitting range</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Range2M</name><description>? Maximum value of second fitting range</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Range3m</name><description>? Minimum value of third fitting range</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Range3M</name><description>? Maximum value of third fitting range</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mue</name><description>? Bulge effective surface brightness in V band</description><unit>mag.arcsec**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>re</name><description>? 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Disk hole radius</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rms</name><description>Unweighted rms deviation of the fit in V band</description><unit>mag.arcsec**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Seeing</name><description>Seeing in arcseconds from the PANBG</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>mu0e</name><description>? Fully corrected bulge effective surface brightness in V band</description><unit>mag.arcsec**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r0e</name><description>? Fully corrected bulge effective radius</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Notes</name><description>[A-J,? ] Notes about individual galaxies (1)</description><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension J2000 (hours) (2)</description></column><column><name>DEJ2000</name><description>Declination J2000 (degrees) (2)</description></column></table><table><name>J/AJ/116/1626/table3</name><description>Parameter fractional errors</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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