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, Nigel Bannister, Joao Bento, Matthew Burleigh, Juan Cabrera, Philipp Eigmüller, Anders Erikson, Ludovic Genolet, Michael Goad, Andrew Grange, Andrés Jordán, Katherine Lawrie, James McCormac & 2 others Marion Neveu, Simon Walker

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution

6 Citations (Scopus)

Abstract

The 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.

Original languageEnglish
Title of host publicationExploring the formation and evolution of planetary systems
Place of PublicationCambridge
PublisherCambridge University Press
Pages311-312
Number of pages2
ISBN (Print)9781107045200
DOIs
Publication statusPublished - 2013

Publication series

NameProceedings of the International Astronomical Union
NumberS299
Volume8
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • Instrumentation: photometers
  • Planetary systems
  • Surveys
  • Techniques: photometric
  • Telescopes

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