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<ri:Resource created="2020-04-15T11:51:59Z" 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>Extended Aperture Photometry of K2 RR Lyrae stars</title><shortName>J/ApJS/244/32</shortName><identifier>ivo://CDS.VizieR/J/ApJS/244/32</identifier><altIdentifier>doi:10.26093/cds/vizier.22440032</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Plachy E.</name></creator><creator><name>Molnar L.</name></creator><creator><name>Bodi A.</name></creator><creator><name>Skarka M.</name></creator><creator><name>Szabo P.</name></creator><creator><name>Szabo R.</name></creator><creator><name>Klagyivik P.,Sodor A.</name></creator><creator><name>Pope B.J.S.</name></creator><date role="Updated">2021-09-09T12:26:53Z</date><date role="Created">2020-04-15T11:51:59Z</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>population-ii-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>The Kepler Space Telescope observed thousands of RR Lyrae stars in the K2 mission. In this paper, we present our photometric solutions using extended apertures in order to conserve the flux of the stars to the highest possible extent. With this method, we are able to avoid most of the problems that RR Lyrae light curves produced by other pipelines suffer from. For post-processing, we apply the K2SC pipeline to our light curves. We provide the EAP (Extended Aperture Photometry) of 432 RR Lyrae stars observed in campaigns 3, 4, 5, and 6. We also provide subclass classifications based on Fourier parameters. We investigated in particular the presence of the Blazhko effect in the stars and found it to be 44.7% among the RRab stars, in agreement with results from independent samples. We found that the amplitude and phase modulation in the Blazhko stars may behave rather differently, at least over the length of a K2 Campaign. We also identified four anomalous Cepheid candidates in the sample, one of which is potentially the first Blazhko-modulated member of its class.</description><source format="bibcode">2019ApJS..244...32P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/244/32</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/V/133">V/133 : Kepler Input Catalog (Kepler, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/598/597">J/ApJ/598/597 : Frequency analysis of fundamental-mode RRL (Alcock+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/1049">J/A+A/430/1049 : RR Gem BV(RI)c differential photometry (Jurcsik+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/391/164">J/MNRAS/391/164 : MW Lyr BV(RI)c light curves (Jurcsik+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/415/1577">J/MNRAS/415/1577 : CoRoT 105288363 Blazhko modulation (Guggenberger+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/61/1">J/AcA/61/1 : VI LCs of Galactic Bulge RR Lyrae (Soszynski+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/31">J/ApJS/213/31 : Blazhko effect from 4yr of Kepler data (Benko+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/64/177">J/AcA/64/177 : VI LCs of Galactic Bulge RR Lyrae (Soszynski+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/579/A19">J/A+A/579/A19 : K2 Variable Catalogue (Armstrong+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/4283">J/MNRAS/452/4283 : 33 RR Lyrae observed in Pisces with K2-E2 (Molnar+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/65/233">J/AcA/65/233 : OGLE Magellanic Clouds anomalous Cepheids (Soszynski+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/456/2260">J/MNRAS/456/2260 : K2 Variability Catalogue II (Armstrong+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/594/A100">J/A+A/594/A100 : K2 new planetary and EB candidates (Barros+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/466/2602">J/MNRAS/466/2602 : Blazhko effect in Galactic RR Lyrae (Prudil+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/67/297">J/AcA/67/297 : OGLE Gal. center Cepheids and RR Lyrae 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