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dc.contributor.authorFeng, Fen_US
dc.contributor.authorTuomi, Men_US
dc.contributor.authorJones, HRAen_US
dc.contributor.authorBarnes, Jen_US
dc.contributor.authorAnglada-Escude, Gen_US
dc.contributor.authorVogt, SSen_US
dc.contributor.authorButler, RPen_US
dc.date.accessioned2018-01-12T11:20:12Z
dc.date.available2017-07-31en_US
dc.date.issued2017-10en_US
dc.date.submitted2018-01-04T10:02:15.737Z
dc.identifier.issn0004-6256en_US
dc.identifier.otherARTN 135en_US
dc.identifier.otherARTN 135en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/31276
dc.relation.ispartofASTRONOMICAL JOURNALen_US
dc.rightsOriginal content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
dc.subjectmethods: numericalen_US
dc.subjectmethods: statisticalen_US
dc.subjectstars: individual (HD 10700)en_US
dc.subjecttechniques: radial velocitiesen_US
dc.titleColor Difference Makes a Difference: Four Planet Candidates around tau Cetien_US
dc.typeArticle
dc.rights.holder© 2017. The American Astronomical Society.
dc.identifier.doi10.3847/1538-3881/aa83b4en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000409393800005&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue4en_US
pubs.notesNo embargoen_US
pubs.publication-statusPublisheden_US
pubs.volume154en_US
qmul.funderAstronomy Research at Queen Mary::Science and Technology Facilities Councilen_US


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