Next Generation Transit Survey (NGTS)

dc.contributor.authorWheatley, Peter J.
dc.contributor.authorPollacco, Don L.
dc.contributor.authorQueloz, Didier
dc.contributor.authorRauer, Heike
dc.contributor.authorWatson, Christopher A.
dc.contributor.authorWest, Richard G.
dc.contributor.authorChazelas, Bruno
dc.contributor.authorLouden, Tom M.
dc.contributor.authorBannister, Nigel
dc.contributor.authorBento, Joao
dc.contributor.authorBurleigh, Matthew
dc.contributor.authorCabrera, Juan
dc.contributor.authorEigmüller, Philipp
dc.contributor.authorErikson, Anders
dc.contributor.authorGenolet, Ludovic
dc.contributor.authorGoad, Michael
dc.contributor.authorGrange, Andrew
dc.contributor.authorJordán, Andrés
dc.contributor.authorLawrie, Katherine
dc.contributor.authorMcCormac, James
dc.contributor.authorNeveu, Marion
dc.contributor.authorWalker, Simon
dc.date.accessioned2017-11-27T13:14:37Z
dc.date.available2017-11-27T13:14:37Z
dc.date.issued2013
dc.descriptionDieser Beitrag ist mit Zustimmung des Rechteinhabers aufgrund einer (DFG geförderten) Allianz- bzw. Nationallizenz frei zugänglich.de
dc.descriptionThis publication is with permission of the rights owner freely accessible due to an Alliance licence and a national licence (funded by the DFG, German Research Foundation) respectively.en
dc.description.abstractThe Next Generation Transit Survey (NGTS) is a new ground-based survey for transiting exoplanets. Our primary goal is to find the first statistically-significant sample of Neptunes and super-Earths that are bright enough for radial velocity confirmation. By measuring precise masses and radii we will constrain the bulk composition and internal structure of planets that span the transition between the gas giants and terrestrial planets. Our brightest exoplanets will also be suitable for atmospheric characterisation with large facilities such as the VLT, JWST and the E-ELT. NGTS construction began in June 2013, and the survey is due to commence in 2014.en
dc.identifier.eissn1743-9221
dc.identifier.issn1743-9213
dc.identifier.urihttps://depositonce.tu-berlin.de/handle/11303/7186
dc.identifier.urihttp://dx.doi.org/10.14279/depositonce-6461
dc.language.isoen
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subject.ddc520 Astronomie und zugeordnete Wissenschaften
dc.subject.ddc526 Mathematische Geografiede
dc.subject.otherplanetary systemsen
dc.subject.otherphotometersen
dc.subject.otherphotometricen
dc.subject.othertelescopesen
dc.subject.othersurveysen
dc.titleNext Generation Transit Survey (NGTS)en
dc.typeArticle
dc.type.versionpublishedVersion
dcterms.bibliographicCitation.doi10.1017/s1743921313008740
dcterms.bibliographicCitation.journaltitleProceedings of the International Astronomical Union
dcterms.bibliographicCitation.originalpublishernameCambridge University Press
dcterms.bibliographicCitation.originalpublisherplaceCambridge
dcterms.bibliographicCitation.pageend312
dcterms.bibliographicCitation.pagestart311
dcterms.bibliographicCitation.volume8
tub.accessrights.dnbdomain
tub.affiliationFak. 2 Mathematik und Naturwissenschaften::Zentrum für Astronomie und Astrophysikde
tub.affiliation.facultyFak. 2 Mathematik und Naturwissenschaftende
tub.affiliation.instituteZentrum für Astronomie und Astrophysikde
tub.publisher.universityorinstitutionTechnische Universität Berlin

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