| dc.contributor.author | Moretti, M. I. | |
| dc.contributor.author | Clementini, G. | |
| dc.contributor.author | Ripepi, V. | |
| dc.contributor.author | Marconi, M. | |
| dc.contributor.author | Rubele, S. | |
| dc.contributor.author | Cioni, M. R L | |
| dc.contributor.author | Muraveva, T. | |
| dc.contributor.author | Groenewegen, M. A T | |
| dc.contributor.author | Cross, N. J G | |
| dc.contributor.author | Ivanov, V. D. | |
| dc.contributor.author | Piatti, A. E. | |
| dc.contributor.author | de Grijs, R. | |
| dc.date.accessioned | 2016-12-19T11:41:22Z | |
| dc.date.available | 2016-12-19T11:41:22Z | |
| dc.date.issued | 2016-06-21 | |
| dc.identifier.citation | Moretti , M I , Clementini , G , Ripepi , V , Marconi , M , Rubele , S , Cioni , M R L , Muraveva , T , Groenewegen , M A T , Cross , N J G , Ivanov , V D , Piatti , A E & de Grijs , R 2016 , ' The VMC survey - XX. Identification of new Cepheids in the Small Magellanic Cloud ' , Monthly Notices of the Royal Astronomical Society , vol. 459 , no. 2 , pp. 1687-1697 . https://doi.org/10.1093/mnras/stw716 | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | PURE: 10505979 | |
| dc.identifier.other | PURE UUID: 8a64cb89-98a4-4b1a-bd0b-a57677c3a0c5 | |
| dc.identifier.other | Scopus: 84974603310 | |
| dc.identifier.uri | http://hdl.handle.net/2299/17445 | |
| dc.description | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © : 2016 M. I. Moretti, et al., Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | |
| dc.description.abstract | We present Ks-band light curves for 299 Cepheids in the Small Magellanic Cloud (SMC) of which 288 are new discoveries that we have identified using multi-epoch near-infrared photometry obtained by the VISTA survey of the Magellanic Clouds system (VMC). The new Cepheids have periods in the range from 0.34 to 9.1 d and cover the magnitude interval 12.9 = 〈Ks〉 = 17.6 mag. Our method was developed using variable stars previously identified by the optical microlensing survey OGLE.We focus on searching newCepheids in external regions of the SMC for which complete VMC Ks-band observations are available and no comprehensive identification of different types of variable stars from other surveys exists yet. | en |
| dc.format.extent | 11 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.subject | Magellanic Clouds | |
| dc.subject | Methods: data analysis | |
| dc.subject | Stars: variables: Cepheids | |
| dc.subject | Surveys | |
| dc.subject | Space and Planetary Science | |
| dc.subject | Astronomy and Astrophysics | |
| dc.title | The VMC survey - XX. Identification of new Cepheids in the Small Magellanic Cloud | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.description.status | Peer reviewed | |
| dc.identifier.url | http://www.scopus.com/inward/record.url?scp=84974603310&partnerID=8YFLogxK | |
| rioxxterms.version | VoR | |
| rioxxterms.versionofrecord | https://doi.org/10.1093/mnras/stw716 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
