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<ri:Resource created="2023-06-19T08:23:09Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Radial velocity data of sigma Dra and HIP 36616</title><shortName>J/A+A/674/A164</shortName><identifier>ivo://CDS.VizieR/J/A+A/674/A164</identifier><altIdentifier>doi:10.26093/cds/vizier.36740164</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Heeren P.</name></creator><creator><name>Tronsgaard R.</name></creator><creator><name>Grundahl F.</name></creator><creator><name>Reffert S.</name></creator><creator><name>Quirrenbach A.,Palle P.L.</name></creator><date role="Updated">2024-11-06T20:04:25Z</date><date role="Created">2023-06-19T08:23:09Z</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>spectroscopic-binary-stars</subject><subject>giant-stars</subject><subject>k-stars</subject><subject>exoplanets</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><description>For existing and future projects dedicated to measuring precise RVs, we have created an open-source, flexible data reduction software to extract RVs from echelle spectra via the I2 cell method. The software, called pyodine, is completely written in Python and has been built in a modular structure to allow for easy adaptation to different instruments. We adapted pyodine to several instruments, two of them being the Hertzsprung SONG located at Teide Observatory (SONG hereafter), and the Hamilton spectrograph at Lick Observatory (Lick hereafter). Both for SONG and Lick data, the pyodine results generally match the RV precision achieved by the dedicated instrument pipelines. Notably, results from our code confirm the planet-induced RV variations of the star HIP 36616 on spectra from SONG and Lick. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>JD</name><description>Julian date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>Radial velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RV</name><description>Error in radial velocity</description><unit>m/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/674/A164/sdra_py</name><description>RV data of sigma Dra, computed with pyodine from Hertzsprung SONG spectra</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>JD</name><description>Julian date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>Radial velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RV</name><description>Error in radial velocity</description><unit>m/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/674/A164/hip_lick</name><description>RV data of HIP 36616, computed with pyodine from spectra from Lick Observatory</description><column><name>RV</name><description>Radial velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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