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dc.contributor.authorTsapras, Yiannis
dc.contributor.authorStreet, Rachel A.
dc.contributor.authorHundertmark, Markus
dc.contributor.authorBachelet, Etienne
dc.contributor.authorDominik, Martin
dc.contributor.authorBozza, Valerio
dc.contributor.authorCassan, Arnaud
dc.contributor.authorWambsganss, Joachim
dc.contributor.authorHorne, Keith Douglas
dc.contributor.authorMao, Shude
dc.contributor.authorZang, Weichen
dc.contributor.authorBramich, Daniel M.
dc.contributor.authorSaha, Abhijit
dc.date.accessioned2020-10-10T23:35:28Z
dc.date.available2020-10-10T23:35:28Z
dc.date.issued2019-12
dc.identifier.citationTsapras , Y , Street , R A , Hundertmark , M , Bachelet , E , Dominik , M , Bozza , V , Cassan , A , Wambsganss , J , Horne , K D , Mao , S , Zang , W , Bramich , D M & Saha , A 2019 , ' ROME/REA : a gravitational microlensing search for exoplanets beyond the snow line on a global network of robotic telescopes ' , Publications of the Astronomical Society of the Pacific , vol. 131 , no. 1006 , 1244401 , pp. 1-12 . https://doi.org/10.1088/1538-3873/ab3b19en
dc.identifier.issn0004-6280
dc.identifier.otherPURE: 261744312
dc.identifier.otherPURE UUID: 70968596-5b42-4b19-954b-cd613fc27dd9
dc.identifier.otherORCID: /0000-0002-3202-0343/work/75996775
dc.identifier.otherWOS: 000503503700001
dc.identifier.urihttp://hdl.handle.net/10023/20760
dc.descriptionFunding: KH acknowledges support from STFC grant ST/R000824/1.en
dc.description.abstractPlanet population synthesis models predict an abundance of planets with semimajor axes between 1 and 10 au, yet they lie at the edge of the detection limits of most planet finding techniques. Discovering these planets and studying their distribution is critical to understanding the physical processes that drive planet formation. ROME/REA is a gravitational microlensing project whose main science driver is to discover exoplanets in the cold outer regions of planetary systems. To achieve this, it uses a novel approach combining a multiband survey with reactive follow-up observations, exploiting the unique capabilities of the Las Cumbres Observatory global network of robotic telescopes combined with a Target and Observation Manager system. We present the main science objectives and a technical overview of the project, including initial results.
dc.format.extent12
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen
dc.rightsCopyright © 2019 The Astronomical Society of the Pacific. All rights reserved. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the author created accepted manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1088/1538-3873/ab3b19en
dc.subjectGalaxy: bulgeen
dc.subjectGravitational lensing: microen
dc.subjectMethods: data analysisen
dc.subjectMethods: observationalen
dc.subjectPlanetary systemsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleROME/REA : a gravitational microlensing search for exoplanets beyond the snow line on a global network of robotic telescopesen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.1088/1538-3873/ab3b19
dc.description.statusPeer revieweden
dc.date.embargoedUntil2020-10-11


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