Liam Raynard
NGTS-2b: An inflated hot-Jupiter transiting a bright F-dwarf
Raynard, Liam; Goad, Michael R.; Gillen, Edward; Nielsen, Louise D.; Watson, Christopher A.; Thompson, Andrew P. G.; McCormac, James; Bayliss, Daniel; Soto, Maritza; Csizmadia, Szilard; Chaushev, Alexander; Burleigh, Matthew R.; Alexander, Richard; Armstrong, David J.; Bouchy, Francois; Briegal, Joshua T.; Cabrera, Juan; Casewell, Sarah L.; Chazelas, Bruno; Cooke, Benjamin F.; Eigmueller, Philipp; Erikson, Anders; Gansicke, Boris T.; Grange, Andrew; Gunther, Maximilian N.; Hodgkin, Simon T.; Hooton, Matthew J.; Jenkins, James S.; Lambert, Gregory; Louden, Tom; Metrailler, Lionel; Moyano, Maximiliano; Pollacco, Don; Poppenhaeger, Katja; Queloz, Didier; Raddi, Roberto; Rauer, Heike; Read, Andrew M.; Smalley, Barry; Smith, Alexis M. S.; Turner, Oliver; Udry, Stephane; Walker, Simon. R.; West, Richard G.; Wheatley, Peter J.
Authors
Michael R. Goad
Edward Gillen
Louise D. Nielsen
Christopher A. Watson
Andrew P. G. Thompson
James McCormac
Daniel Bayliss
Maritza Soto
Szilard Csizmadia
Alexander Chaushev
Matthew R. Burleigh
Richard Alexander
David J. Armstrong
Francois Bouchy
Joshua T. Briegal
Juan Cabrera
Sarah L. Casewell
Bruno Chazelas
Benjamin F. Cooke
Philipp Eigmueller
Anders Erikson
Boris T. Gansicke
Andrew Grange
Maximilian N. Gunther
Simon T. Hodgkin
Matthew J. Hooton
James S. Jenkins
Gregory Lambert
Tom Louden
Lionel Metrailler
Maximiliano Moyano
Don Pollacco
Katja Poppenhaeger
Didier Queloz
Roberto Raddi
Heike Rauer
Andrew M. Read
Barry Smalley b.smalley@keele.ac.uk
Alexis M. S. Smith
Oliver Turner
Stephane Udry
Simon. R. Walker
Richard G. West
Peter J. Wheatley
Abstract
We report the discovery of NGTS-2b, an inflated hot-Jupiter transiting a bright F5V star (2MASS J14202949 - 3112074; Teff = 6478+94-89 K), discovered as part of the Next Generation Transit Survey (NGTS). The planet is in a P = 4.51?d orbit with mass 0.74+0.13-0.12MJ, radius 1.595+0.047-0.045RJ, and density 0.226+0.040-0.038 g?cm-3; therefore one of the lowest density exoplanets currently known. With a relatively deep 1.0 per cent transit around a bright V = 10.96 host star, NGTS-2b is a prime target for probing giant planet composition via atmospheric transmission spectroscopy. The rapid rotation (?v?sin?i = 15.2 ± 0.8?km?s-1) also makes this system an excellent candidate for Rossiter–McLaughlin follow-up observations, to measure the sky-projected stellar obliquity. NGTS-2b was confirmed without the need for follow-up photometry, due to the high precision of the NGTS photometry.
Citation
Raynard, L., Goad, M. R., Gillen, E., Nielsen, L. D., Watson, C. A., Thompson, A. P. G., …Wheatley, P. J. (2018). NGTS-2b: An inflated hot-Jupiter transiting a bright F-dwarf. Monthly Notices of the Royal Astronomical Society, 481(4), 4960-4970. https://doi.org/10.1093/mnras/sty2581
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 17, 2018 |
Publication Date | Dec 21, 2018 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Volume | 481 |
Issue | 4 |
Pages | 4960-4970 |
DOI | https://doi.org/10.1093/mnras/sty2581 |
Keywords | techniques, photometric, stars:individual: NGTS-2, planetary systems |
Publisher URL | http://dx.doi.org/10.1093/mnras/sty2581 |
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