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<ri:Resource created="2026-07-27T10:48:53Z" status="active" updated="2026-09-16T07:26:12Z" 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>Andromeda XXV new member stars kinematics</title><shortName>J/MNRAS/521/3527</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/521/3527</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Charles E.J.E.</name></creator><creator><name>Collins M.L.M.</name></creator><creator><name>Rich R.M.</name></creator><creator><name>Read J.I.</name></creator><creator><name>Kim S.Y.</name></creator><creator><name>Ibata R.A.,Martin N.F.</name></creator><creator><name>Chapman S.C.</name></creator><creator><name>Balbinot E.</name></creator><creator><name>Weisz D.R.</name></creator><date role="Updated">2026-09-16T07:26:12Z</date><date role="Created">2026-07-27T10:48:53Z</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>dwarf-galaxies</subject><subject>galaxies</subject><subject>galaxy-kinematics</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Andromeda (And) XXV has previously been reported as a dwarf spheroidal galaxy (dSph) with little-to-no dark matter. However, the uncertainties on this result were significant. In this study, we nearly double the number of member stars and re-derive the kinematics and mass of And XXV. We find that And XXV has a systemic velocity of v_r_ = -107.7 +/- 1.0 km/s and a velocity dispersion of {sigma}_v_ = 3.7^+1.2^_-1.1_ km/s. With this updated velocity dispersion and a new literature measurement of the radial surface brightness profile, we derive a mass contained within the half-light radius of M(r &lt; r_h_) = 4.79^+3.0^_-2.9_ * 10^6^ M_{sun}_. This mass corresponds to a mass-to-light ratio of [M/L]_rh_ = 25^+17^_-16_ M_{sun}_/L_{sun}_, demonstrating that And XXV is most-likely dark matter dominated. We also measure the metallicity of And XXV to be [Fe/H] = -1.9 +/- 0.1 dex, which is in agreement with previous results. Finally, we extend the analysis of And XXV to include mass modelling using GravSphere. We find that And XXV has a low central dark matter density, {rho}_DM_(150 pc) = 2.3^+1.4^_-1.1_ * 10^7^ M_{sun}_ kpc^-3^, which makes And XXV a clear outlier when compared to other local group dSphs of the similar stellar mass. In a companion paper, we will explore whether some combination of dark matter cusp-core transformations and/or tides can explain And XXV's low density.</description><source format="bibcode">2023MNRAS.521.3527C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/521/3527</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/491/3496">J/MNRAS/491/3496 : Andromeda XIX member stars (Collins+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/488/2743">J/MNRAS/488/2743 : Giant Galactic dwarf satellite in Gaia DR2 (Torrealba+,2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/485/2010">J/MNRAS/485/2010 : Kinematics of the Tucana Dwarf Galaxy (Gregory+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/380/281">J/MNRAS/380/281 : Faint galactic satellites spectroscopic survey</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/895/78">J/ApJ/895/78 : [Fe/H] and [{alpha}/Fe] in M31 dwarf galaxies (Wojno+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/11">J/ApJ/883/11 : Magellan/IMACS spectra of Crater II &amp; Hercules (Fu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/11">J/ApJ/838/11 : Member stars in the MW satellite Tucana III (Simon+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/83">J/ApJ/838/83 : Radial velocities, abundances &amp; membership in TriII</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/167">J/ApJ/833/167 : PAndAS view of Andromeda satellites. 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