The Next Generation Transit Survey (NGTS)

Peter J. Wheatley, Don L. Pollacco, Didier Queloz, Heike Rauer, Christopher A. Watson, Richard G. West, Bruno Chazelas, Tom M. Louden, Simon Walker, Nigel Bannister, Joao Bento, Matthew Burleigh, Juan Cabrera, Philipp Eigmüller, Anders Erikson, Ludovic Genolet, Michael Goad, Andrew Grange, Andrés Jordán, Katherine LawrieJames McCormac, Marion Neveu

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contributionpeer-review

64 Citations (Scopus)
7 Downloads (Pure)


The Next Generation Transit Survey (NGTS) is a new ground-based sky survey designed to find transiting Neptunes and super-Earths. By covering at least sixteen times the sky area of Kepler, we will find small planets around stars that are sufficiently bright for radial velocity confirmation, mass determination and atmospheric characterisation. The NGTS instrument will consist of an array of twelve independently pointed 20 cm telescopes fitted with red-sensitive CCD cameras. It will be constructed at the ESO Paranal Observatory, thereby benefiting from the very best photometric conditions as well as follow up synergy with the VLT and E-ELT. Our design has been verified through the operation of two prototype instruments, demonstrating white noise characteristics to sub-mmag photometric precision. Detailed simulations show that about thirty bright super-Earths and up to two hundred Neptunes could be discovered. Our science operations are due to begin in 2014.

Original languageEnglish
Title of host publicationHot planets and cool stars
EditorsRoberto Saglia
Place of PublicationLes Ulis, France
PublisherEDP Sciences
Number of pages4
ISBN (Print)9782759809851
Publication statusPublished - 2013
Externally publishedYes
EventConference on Hot Planets and Cool Stars - Garching, Germany
Duration: 12 Nov 201216 Nov 2012

Publication series

NameEPJ Web of Conferences
PublisherEDP Sciences
ISSN (Electronic)2100-014X


OtherConference on Hot Planets and Cool Stars

Bibliographical note

Copyright 2013 by the authors, published by EDP Sciences. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.


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