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<ri:Resource created="2022-05-12T08:40:46Z" 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>The EXPRES Stellar Signals Project. II. RVel</title><shortName>J/AJ/163/171</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/171</identifier><altIdentifier>doi:10.26093/cds/vizier.51630171</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhao L.L.</name></creator><creator><name>Fischer D.A.</name></creator><creator><name>Ford E.B.</name></creator><creator><name>Wise A.</name></creator><creator><name>Cretignier M.</name></creator><creator><name>Aigrain S.,Barragan O.</name></creator><creator><name>Bedell M.</name></creator><creator><name>Buchhave L.A.</name></creator><creator><name>Camacho J.D.</name></creator><creator><name>Cegla H.M.,Cisewski-Kehe J.</name></creator><creator><name>Collier Cameron A.</name></creator><creator><name>de Beurs Z.L.</name></creator><creator><name>Dodson-Robinson S.,Dumusque X.</name></creator><creator><name>Faria J.P.</name></creator><creator><name>Gilbertson C.</name></creator><creator><name>Haley C.</name></creator><creator><name>Harrell J.</name></creator><creator><name>Hogg D.W.,Holzer P.</name></creator><creator><name>John A.A.</name></creator><creator><name>Klein B.</name></creator><creator><name>Lafarga M.</name></creator><creator><name>Lienhard F.</name></creator><creator><name>Maguire-Rajpaul V.,Mortier A.</name></creator><creator><name>Nicholson B.</name></creator><creator><name>Palumbo M.L.</name></creator><creator><name>Ramirez Delgado V.</name></creator><creator><name>Shallue C.J.,Vanderburg A.</name></creator><creator><name>Viana P.T.P.</name></creator><creator><name>Zhao J.</name></creator><creator><name>Zicher N.</name></creator><creator><name>Cabot S.H.C.</name></creator><creator><name>Henry G.W.,Roettenbacher R.M.</name></creator><creator><name>Brewer J.M.</name></creator><creator><name>Llama J.</name></creator><creator><name>Petersburg R.R.</name></creator><creator><name>Szymkowiak A.E.</name></creator><date role="Updated">2022-09-30T22:19:07Z</date><date role="Created">2022-05-12T08:40:46Z</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>exoplanets</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>Measured spectral shifts due to intrinsic stellar variability (e.g., pulsations, granulation) and activity (e.g., spots, plages) are the largest source of error for extreme-precision radial-velocity (EPRV) exoplanet detection. Several methods are designed to disentangle stellar signals from true center-of-mass shifts due to planets. The Extreme-precision Spectrograph (EXPRES) Stellar Signals Project (ESSP) presents a self-consistent comparison of 22 different methods tested on the same extreme-precision spectroscopic data from EXPRES. Methods derived new activity indicators, constructed models for mapping an indicator to the needed radial-velocity (RV) correction, or separated out shape- and shift-driven RV components. Since no ground truth is known when using real data, relative method performance is assessed using the total and nightly scatter of returned RVs and agreement between the results of different methods. Nearly all submitted methods return a lower RV rms than classic linear decorrelation, but no method is yet consistently reducing the RV rms to sub-meter-per-second levels. There is a concerning lack of agreement between the RVs returned by different methods. These results suggest that continued progress in this field necessitates increased interpretability of methods, high-cadence data to capture stellar signals at all timescales, and continued tests like the ESSP using consistent data sets with more advanced metrics for method performance. Future comparisons should make use of various well-characterized data sets-such as solar data or data with known injected planetary and/or stellar signals-to better understand method performance and whether planetary signals are preserved.</description><source format="bibcode">2022AJ....163..171Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/171</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/ApJ/457/L99">J/ApJ/457/L99 : 25yr CaII-HK observations F-K nearby stars (Baliunas+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/141/503">J/ApJS/141/503 : Radial Velocities for 889 late-type stars (Nidever+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/495/959">J/A+A/495/959 : Radial velocity curve of HD 189733 (Boisse+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/303">J/A+A/506/303 : CoRoT-7 radial velocities (Queloz+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/725/875">J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/535/A55">J/A+A/535/A55 : 4 stars with long-period planets (Dumusque+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/101">J/ApJ/746/101 : Diameters and temperatures of AFG stars (Boyajian+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A61">J/A+A/560/A61 : A frequency Comb calibrated solar atlas (Molaro+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A79">J/A+A/551/A79 : Radial velocity period variations in {tau}Ceti (Tuomi+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/A35">J/A+A/566/A35 : Radial velocities of HD 41248 (Santos+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/32">J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/593/A5">J/A+A/593/A5 : Radial velocity fitting challenge dataset (Dumusque, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/472/1618">J/MNRAS/472/1618 : Kepler study of starspot lifetimes (Giles+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/607/A124">J/A+A/607/A124 : K-G-F dwarfs stellar granulation variability (Meunier+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/474/2094">J/MNRAS/474/2094 : Inferring probabilistic stellar rot periods (Angus+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/126">J/AJ/155/126 : Radial velocities &amp; photometry of Kdwarf HD26965 (Diaz+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/636/A36">J/A+A/636/A36 : Absolute radial velocities CARMENES M dwarfs (Lafarga+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/187">J/AJ/159/187 : 1st RVs with EXPRES spectrograph: 51Peg (Petersburg+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/639/A77">J/A+A/639/A77 : Proxima Cen RV, FWHM and fluxes (Suarez Mascareno+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/26">J/AJ/161/26 : EXPRES II HD101501 photometry &amp; radial velocity (Cabot+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/80">J/AJ/161/80 : Excalibur calib. method HD34411 RVs with EXPRESS (Zhao+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/19">J/AJ/163/19 : EXPRES III. 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