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dc.contributor.authorMasters, Karen L.
dc.contributor.authorStark, David V.
dc.contributor.authorPace, Zachary J.
dc.contributor.authorPhipps, Frederika
dc.contributor.authorRujopakarn, Wiphu
dc.contributor.authorSamanso, Nattida
dc.contributor.authorHarrington, Emily
dc.contributor.authorSánchez-Gallego, José R.
dc.contributor.authorAvila-Reese, Vladimir
dc.contributor.authorBershady, Matthew
dc.contributor.authorCherinka, Brian
dc.contributor.authorFielder, Catherine E.
dc.contributor.authorFinnegan, Daniel
dc.contributor.authorRiffel, Rogemar A.
dc.contributor.authorRowlands, Kate
dc.contributor.authorShamsi, Shoaib
dc.contributor.authorNewnham, Lucy
dc.contributor.authorWeijmans, Anne-Marie
dc.contributor.authorWitherspoon, Catherine A.
dc.identifier.citationMasters , K L , Stark , D V , Pace , Z J , Phipps , F , Rujopakarn , W , Samanso , N , Harrington , E , Sánchez-Gallego , J R , Avila-Reese , V , Bershady , M , Cherinka , B , Fielder , C E , Finnegan , D , Riffel , R A , Rowlands , K , Shamsi , S , Newnham , L , Weijmans , A-M & Witherspoon , C A 2019 , ' H I - MaNGA : H I follow-up for the MaNGA survey ' , Monthly Notices of the Royal Astronomical Society , vol. 488 , no. 3 , pp. 3396-3405 .
dc.identifier.otherPURE: 260532117
dc.identifier.otherPURE UUID: 9d4fe711-2824-4c89-8c6d-56462e8bfee6
dc.identifier.otherBibCode: 2019MNRAS.488.3396M
dc.identifier.otherORCID: /0000-0002-5908-6852/work/60630867
dc.identifier.otherScopus: 85075147615
dc.identifier.otherWOS: 000485158400031
dc.description.abstractWe present the H I-MaNGA programme of H I follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey. MaNGA, which is part of the Fourth phase of the Sloan Digital Sky Surveys, is in the process of obtaining integral field unit spectroscopy for a sample of ∼10 000 nearby galaxies. We give an overview of the H I 21cm radio follow-up observing plans and progress and present data for the first 331 galaxies observed in the 2016 observing season at the Robert C. Bryd Green Bank Telescope. We also provide a cross-match of the current MaNGA(DR15) sample with publicly available H I data from the Arecibo Legacy Fast Arecibo L-band Feed Array survey. The addition of H I data to the MaNGA data set will strengthen the survey's ability to address several of its key science goals that relate to the gas content of galaxies, while also increasing the legacy of this survey for all extragalactic science.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2019, the Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. This work has been made available online in accordance with the publisher's policies. This is the author created accepted version manuscript following peer review and as such may differ slightly from the final published version. The final published version of this work is available at
dc.subjectGalaxies: ISMen
dc.subjectRadio lines: galaxiesen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleH I - MaNGA : H I follow-up for the MaNGA surveyen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.Centre for Contemporary Arten
dc.description.statusPeer revieweden

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