I. Apergis, D. Bayliss, S. Ulmer-Moll, S. Gill, T. Rodel, M. Battley, P. Benni, A. Bieryla, J Blake, A. Bonfanti, F. Bouchy, E. M. Bryant, M. Burleigh, S Carlier, S. Casewell, H. Chakraborty, A. Claringbold, K. A. Collins, B. Davies, X. Dumusque, T Edkins, F. Eeles-Nolle, J. A. Egger, J. Fernández Fernández, M. A. F. Keniger, P. Figueira, M. R. Goad, G Harvey, F. Hawthorn, M. J. Hobson, M. Houelle, G. Isopi, T Jestin, A. Kendall, M. Lendl, D. A. Lewis, I. Lockley, F. Mallia, J. McCormac, M. A. Mitchell, L. Mignon, H. P. Osborn, A. Psaridi, A Romanec, S. Saha, A Sedgley, S. G. Sousa, N. Thomas, S. Udry, C. A. Watson, R. G. West, T. Wilson, P. J. Wheatley, J Williams, A Zapparata, K Zielinski
Abstract
We report the discovery and characterization of NGTS-39 b (TIC 453147896 b), a warm Jupiter transiting a Sun-like star on a 58.2 d, eccentric (e = 0.386±0.019) orbit. NGTS-39 b was first identified from a Transiting Exoplanet Survey Satellite single transit event, and subsequently confirmed with NGTS photometry and radial velocity measurements from CORALIE and HARPS. The host star is a bright (Tmag = 11.02) F9 dwarf with effective temperature of Teff = 6053+67−30 K. NGTS-39 b is a Jupiter-sized gas giant with a radius of 1.088±0.012 RJ and a mass of 1.467±0.081 MJ. Its equilibrium temperature is 519+6−5 K, placing it between short-period hot Jupiters and cold, Jupiter-like giants. The high orbital eccentricity and intermediate equilibrium temperature of NGTS-39 b make it a valuable test case for formation and migration models, particularly in the poorly sampled regime of long-period gas giants. The RV data show a linear trend of ˙γ=−17.75 m s−1 yr−1, which indicates the presence of an outer companion. The discovery of NGTS-39 b contributes to the small but growing population of transiting warm Jupiters with P> 50 d orbiting bright stars.
Keywords
planets and satellites: detection / planets and satellites: individual: TIC-453147896 b / techniques: photometric / techniques: radial velocities
Monthly Notices of the Royal Astronomical Society
Volume 550, Issue stag1271, Page 17
2026 August





