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<ri:Resource created="2026-03-05T12:49:33Z" status="active" updated="2026-03-07T00:00:00Z" 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>Colours from low-z LS DR9 galaxies</title><shortName>J/MNRAS/518/3999</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/518/3999</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liao L.-W.</name></creator><creator><name>Cooper A.P.</name></creator><date role="Updated">2026-03-05T12:02:38Z</date><date role="Created">2026-03-05T12:49:33Z</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><subject>visible-astronomy</subject><subject>astrometry</subject><subject>redshifted</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>star-forming-regions</subject><description>Radial colour gradients within galaxies arise from gradients of stellar age, metallicity, and dust reddening. Large samples of colour gradients from wide- area imaging surveys can complement smaller integral-field spectroscopy data sets and can be used to constrain galaxy formation models. Here, we measure colour gradients for low-redshift galaxies (z &lt; 0.1) using photometry from the DESI Legacy Imaging Survey DR9. Our sample comprises ~93000 galaxies with spectroscopic redshifts and ~574000 galaxies with photometric redshifts. We focus on gradients across a radial range 0.5R_eff_ to R_eff_, which corresponds to the inner disc of typical late-type systems at low redshift. This region has been the focus of previous statistical studies of colour gradients and has recently been explored by spectroscopic surveys such as MaNGA. We find that the colour gradients of most galaxies in our sample are negative (redder towards the centre), consistent with the literature. We investigate empirical relationships between colour gradient, average g-r and r-z colour, Mr, M*, and sSFR. Trends of gradient strength with M_r_ (M*) show an inflection around Mr~-21(log_10_M*/M_{Sun}_ ~10.5). Below this mass, colour gradients become steeper with increasing M*, whereas colour gradients in more massive galaxies become shallower. We find that positive gradients (bluer stars at smaller radii) are typical for galaxies of M_*_~10^8^M_{Sun}_. We compare our results to age and metallicity gradients in two data sets derived from fits of different stellar population libraries to MaNGA spectra, but find no clear consensus explanation for the trends we observe. Both MaNGA data sets seem to imply a significant contribution from dust reddening, in particular, to explain the flatness of colour gradients along the red sequence.</description><source format="bibcode">2023MNRAS.518.3999L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/518/3999</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/506/928">J/MNRAS/506/928 : Stellar mass-size relation for low M* galaxies</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/491/3562">J/MNRAS/491/3562 : CALIFA ETGs spatially resolved stellar pop. (Zibetti+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/483/1862">J/MNRAS/483/1862 : Metallicity gradient across the Hubble sequence</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/476/1765">J/MNRAS/476/1765 : MaNGA E and S galaxies properties (Li+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/703">J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/581/A103">J/A+A/581/A103 : CALIFA survey across the Hubble sequence (Gonzalez+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/313/377">J/A+A/313/377 : Near-IR photometry of 86 galaxies. IV. (de Jong 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/907/85">J/ApJ/907/85 : The SAGA Survey. II. Satellite systems around galaxies</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/175">J/ApJ/883/175 : First release of the MaNGA Stellar Library (MaStar)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/766/109">J/ApJ/766/109 : Color/age/metallicity gradients of E galaxies (Kim+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/527/573">J/ApJ/527/573 : Line Strengths in Elliptical Galaxies (Kobayashi+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/86">J/AJ/154/86 : MaNGA catalog, DR15 (Wake+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/2471">J/AJ/112/2471 : The Ursa Major cluster. I. 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