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<ri:Resource created="2021-05-25T13:46:27Z" 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>List of 100 targets for the NEID Earth Twin Survey</title><shortName>J/AJ/161/130</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/130</identifier><altIdentifier>doi:10.26093/cds/vizier.51610130</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gupta A.F.</name></creator><creator><name>Wright J.T.</name></creator><creator><name>Robertson P.</name></creator><creator><name>Halverson S.</name></creator><creator><name>Luhn J.</name></creator><creator><name>Roy A.,Mahadevan S.</name></creator><creator><name>Ford E.B.</name></creator><creator><name>Bender C.F.</name></creator><creator><name>Blake C.H.</name></creator><creator><name>Hearty F.</name></creator><creator><name>Kanodia S.,Logsdon S.E.</name></creator><creator><name>McElwain M.W.</name></creator><creator><name>Monson A.</name></creator><creator><name>Ninan J.P.</name></creator><creator><name>Schwab C.,Stefansson G.</name></creator><creator><name>Terrien R.C.</name></creator><date role="Updated">2022-09-30T21:47:42Z</date><date role="Created">2021-05-25T13:46:27Z</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>surveys</subject><subject>exoplanets</subject><subject>dwarf-stars</subject><subject>visible-astronomy</subject><subject>effective-temperature</subject><description>NEID is a high-resolution optical spectrograph on the WIYN 3.5m telescope at Kitt Peak National Observatory and will soon join the new generation of extreme precision radial velocity instruments in operation around the world. We plan to use the instrument to conduct the NEID Earth Twin Survey (NETS) over the course of the next 5 years, collecting hundreds of observations of some of the nearest and brightest stars in an effort to probe the regime of Earth-mass exoplanets. Even if we take advantage of the extreme instrumental precision conferred by NEID, it will be difficult to disentangle the weak (~10cm/s) signals induced by such low-mass, long-period exoplanets from stellar noise for all but the quietest host stars. In this work, we present a set of quantitative selection metrics which we use to identify an initial NETS target list consisting of stars conducive to the detection of exoplanets in the regime of interest. We also outline a set of observing strategies with which we aim to mitigate uncertainty contributions from intrinsic stellar variability and other sources of noise.</description><source format="bibcode">2021AJ....161..130G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/130</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/other/Sci/330.653">J/other/Sci/330.653 : Detected planets in the Eta-Earth Survey (Howard+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/804/64">J/ApJ/804/64 : Empirical and model parameters of 183 M dwarfs (Mann+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A72">J/A+A/584/A72 : Transiting rocky planet at 6.5pc from the Sun (Motalebi+, 2015)</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/AJ/153/208">J/AJ/153/208 : LCES HIRES/Keck radial velocity Exoplanet Survey (Butler+,2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/597/A52">J/A+A/597/A52 : K and G dwarfs stellar granulation variability (Meunier+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/109">J/AJ/158/109 : Occurrence rates of planets orbiting FGK stars (Hsu+, 2019)</relatedResource><relatedResource 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