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

Author(s):
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.; Pérez Hernández, F.; Persson, C.M.; Albrecht, S.H.; Barragán, O.; Cabrera, J.; Cochran, W.D.; Deeg, H.J.; Fridlund, M.; Georgieva, I.Y.; Goffo, E.; Guenther, E.W.; Hatzes, A.P.; Kabath, P.; Livingston, J.H.; Luque, R.; Palle, E.; Redfield, S.; Rodler, F.; Serrano, L.M.; Eylen, V. Van
Published
2022
Publication type
Article / Letter to editor
planetary systemsplanets and satellites detectionplanets and satellites individualK2-99 bplanets and satellitesindividualK2-99 cAstrophysics - Earth and Planetary AstrophysicsAstrophysics - Solar and Stellar Astrophysics
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 510, no. 4, p. 5035-5049
hdl
1887/3561586
doi
10.1093/mnras/stab3497
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.5035S