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Authordc.contributor.authorWheatley, Peter J. 
Authordc.contributor.authorWest, Richard G. 
Authordc.contributor.authorGoad, Michael R. 
Authordc.contributor.authorJenkins, James Stewart 
Authordc.contributor.authorErikson, Anders 
Authordc.contributor.authorSoto, Maritza 
Admission datedc.date.accessioned2018-07-20T19:51:00Z
Available datedc.date.available2018-07-20T19:51:00Z
Publication datedc.date.issued2018
Cita de ítemdc.identifier.citationMonthly Notices of The Royal Astronomical Society 475, 4476–4493 (2018)es_ES
Identifierdc.identifier.other10.1093/mnras/stx2836
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/150108
Abstractdc.description.abstractWe describe the Next Generation Transit Survey (NGTS), which is a ground-based project searching for transiting exoplanets orbiting bright stars. NGTS builds on the legacy of previous surveys, most notably WASP, and is designed to achieve higher photometric precision and hence find smaller planets than have previously been detected from the ground. It also operates in red light, maximizing sensitivity to late K and early M dwarf stars. The survey specifications call for photometric precision of 0.1 per cent in red light over an instantaneous field of view of 100 deg(2), enabling the detection of Neptune-sized exoplanets around Sun-like stars and super-Earths around M dwarfs. The survey is carried out with a purpose-built facility at Cerro Paranal, Chile, which is the premier site of the European Southern Observatory (ESO). An array of twelve 20 cm f/2.8 telescopes fitted with back-illuminated deep-depletion CCD cameras is used to survey fields intensively at intermediate Galactic latitudes. The instrument is also ideally suited to ground-based photometric follow-up of exoplanet candidates from space telescopes such as TESS, Gaia and PLATO. We present observations that combine precise autoguiding and the superb observing conditions at Paranal to provide routine photometric precision of 0.1 per cent in 1 h for stars with I-band magnitudes brighter than 13. We describe the instrument and data analysis methods as well as the status of the survey, which achieved first light in 2015 and began full-survey operations in 2016. NGTS data will be made publicly available through the ESO archive.es_ES
Patrocinadordc.description.sponsorshipUK Science and Technology Facilities Council (STFC) ST/M001962/1 STFC ST/M001962/1 ST/L000733/1 ST/P000495/1 1226157 1490409 European Research Council (ERC) under the European Union's Seventh Framework Programme (FP)/ERC Grant 320964 Qatar National Research Foundation FONDECYT 1161218 1171208 CATA-Basal PB06 Ministry for the Economy, Development, and Tourism's Programa Iniciativa Cientifica Milenio through grant IC 120009 BASAL CATA PFB-06 Ministry for the Economy, Development Tourism's Programa Iniciativa Cientifica Milenio IC 120009 Accordo ASIINAF for PLATO 2015-019-Res_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherOxford University Presses_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceMonthly Notices of The Royal Astronomical Societyes_ES
Keywordsdc.subjectAtmospheric effectses_ES
Keywordsdc.subjectInstrumentation photometerses_ES
Keywordsdc.subjectTechniques photometrices_ES
Keywordsdc.subjectSurveyses_ES
Keywordsdc.subjectPlanets and satellites detectiones_ES
Keywordsdc.subjectPlanetary systemses_ES
Títulodc.titleThe next generation transit survey (NGTS)es_ES
Document typedc.typeArtículo de revistaes_ES
Catalogueruchile.catalogadortjnes_ES
Indexationuchile.indexArtículo de publicación ISIes_ES


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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile