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<ri:Resource created="2018-07-19T13:13:24Z" 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>RR Lyrae candidates in the MW outer halo</title><shortName>J/ApJ/849/150</shortName><identifier>ivo://CDS.VizieR/J/ApJ/849/150</identifier><altIdentifier>doi:10.26093/cds/vizier.18490150</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cohen J.G.</name></creator><creator><name>Sesar B.</name></creator><creator><name>Bahnolzer S.</name></creator><creator><name>He K.</name></creator><creator><name>Kulkarni S.R.</name></creator><creator><name>Prince T.A.,Bellm E.</name></creator><creator><name>Laher R.R.</name></creator><date role="Updated">2019-12-10T06:59:42Z</date><date role="Created">2018-07-19T13:13:24Z</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>variable-stars</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>radial-velocity</subject><subject>stellar-distance</subject><description>RR Lyrae stars are ideal massless tracers that can be used to study the total mass and dark matter content of the outer halo of the Milky Way (MW). This is because they are easy to find in the light-curve databases of large stellar surveys and their distances can be determined with only knowledge of the light curve. We present here a sample of 112 RR Lyr stars beyond 50kpc in the outer halo of the MW, excluding the Sgr streams, for which we have obtained moderate-resolution spectra with Deimos on the Keck II Telescope. Four of these have distances exceeding 100kpc. These were selected from a much larger set of 447 candidate RR Lyr stars that were data-mined using machine-learning techniques applied to the light curves of variable stars in the Palomar Transient Facility database. The observed radial velocities taken at the phase of the variable corresponding to the time of observation were converted to systemic radial velocities in the Galactic standard of rest. From our sample of 112 RR Lyr stars we determine the radial velocity dispersion in the outer halo of the MW to be ~90km/s at 50kpc, falling to about 65km/s near 100 kpc once a small number of major outliers are removed. With reasonable estimates of the completeness of our sample of 447 candidates and assuming a spherical halo, we find that the stellar density in the outer halo declines as r^-4^.</description><source format="bibcode">2017ApJ...849..150C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/849/150</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/I/315">I/315 : UCAC3 Catalogue (Zacharias+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/375/1381">J/MNRAS/375/1381 : Kinematics of RR Lyr and HB stars in NGP (Kinman+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/678/851">J/ApJ/678/851 : RR Lyrae survey in the Galactic Halo (Keller+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/678/865">J/ApJ/678/865 : LONEOS-I RR Lyrae stars (Miceli+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/684/1143">J/ApJ/684/1143 : BHB candidates in the Milky Way (Xue+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/1053">J/ApJ/701/1053 : Abundances of 8 stars in the Draco dSph (Cohen+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4377">J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/59">J/AJ/139/59 : Milky Way halo velocity dispersion profile (Brown+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/719/931">J/ApJ/719/931 : Chemical evolution of the UMi dSph (Cohen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/717">J/ApJ/708/717 : Light curve templates of RR Lyrae stars (Sesar+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/187">J/AJ/142/187 : HST obs. of 7 Pop.II variable stars (Benedict+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/65">J/ApJ/740/65 : VLA search for 5GHz radio transients (Ofek+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/4">J/ApJ/731/4 : Galactic halo as seen by the CFHTLS (Sesar+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/79">J/ApJ/738/79 : SDSS-DR8 BHB stars in the Milky Way's halo (Xue+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/114">J/AJ/144/114 : Radial velocities of 6 field RR Lyrae (Sesar+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/99">J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/23">J/ApJ/756/23 : V-band follow-up of RR Lyrae from SEKBO (Akhter+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/32">J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/776/26">J/ApJ/776/26 : RRab stars in the Orphan stream distances (Sesar+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/21">J/AJ/146/21 : LINEAR. 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