English

The Next Generation Transit Survey (NGTS)

Earth and Planetary Astrophysics 2018-03-14 v1 Instrumentation and Methods for Astrophysics

Abstract

We 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, maximising 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 square degrees, 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 20cm f/2.8 telescopes fitted with back-illuminated deep-depletion CCD cameras are 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 hour 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.

Keywords

Cite

@article{arxiv.1710.11100,
  title  = {The Next Generation Transit Survey (NGTS)},
  author = {Peter J. Wheatley and Richard G. West and Michael R. Goad and James S. Jenkins and Don L. Pollacco and Didier Queloz and Heike Rauer and Stephane Udry and Christopher A. Watson and Bruno Chazelas and Philipp Eigmuller and Gregory Lambert and Ludovic Genolet and James McCormac and Simon Walker and David J. Armstrong and Daniel Bayliss and Joao Bento and Francois Bouchy and Matthew R. Burleigh and Juan Cabrera and Sarah L. Casewell and Alexander Chaushev and Paul Chote and Szilard Csizmadia and Anders Erikson and Francesca Faedi and Emma Foxell and Boris T. Gansicke and Edward Gillen and Andrew Grange and Maximilian N. Gunther and Simon T. Hodgkin and James Jackman and Andres Jordan and Tom Louden and Lionel Metrailler and Maximiliano Moyano and Louise D. Nielsen and Hugh P. Osborn and Katja Poppenhaeger and Roberto Raddi and Liam Raynard and Alexis M. S. Smith and Maritza Soto and Ruth Titz-Weider},
  journal= {arXiv preprint arXiv:1710.11100},
  year   = {2018}
}

Comments

20 pages, 17 Figures, Accepted for publication in MNRAS

R2 v1 2026-06-22T22:30:10.040Z