K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant

Autor: A M S Smith, S N Breton, Sz Csizmadia, F Dai, D Gandolfi, R A García, A W Howard, H Isaacson, J Korth, K W F Lam, S Mathur, G Nowak, F Pérez Hernández, C M Persson, S H Albrecht, O Barragán, J Cabrera, W D Cochran, H J Deeg, M Fridlund, I Y Georgieva, E Goffo, E W Guenther, A P Hatzes, P Kabath, J H Livingston, R Luque, E Palle, S Redfield, F Rodler, L M Serrano, V Van Eylen

Publikováno v: Smith, A M S, Breton, S N, Csizmadia, S, Dai, F, Gandolfi, D, García, R A, Howard, A W, Isaacson, H, Korth, J, Lam, K W F, Mathur, S, Nowak, G, Hernández, F P, Persson, C M, Albrecht, S H, Barragán, O, Cabrera, J, Cochran, W D, Deeg, H J, Fridlund, M, Georgie v a, I Y, Gof fo, E, Guenther, E W, Hatzes, A P, Kabath, P, Livingston, J H, Luque, R, Palle, E, Redfield, S, Rodler, F, Serrano, L M & Van Eylen, V 2022, ' K2-99 revisited : A non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant ', Monthly Notices of the Royal Astronomical Society, vol. 510, no. 4, pp. 5035-5049 . https://doi.org/10.1093/mnras/stab3497
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 510(4), 5035-5049

We report new photometric and spectroscopic observations of the K2-99 planetary system. Asteroseismic analysis of the short-cadence light curve from K2’s Campaign 17 allows us to refine the stellar properties. We find K2-99 to be significantly smal

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51d4ae8314a7e3d93b18759c2e7bf50a