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

Smith, A.M.S.; Breton, S.N.; Csizmadia, S.; Dai, F.; Gandolfi, D.; García, R.A.; ... ; Eylen, V. Van (2022)

Article / Letter to editor

• planetary systems
• planets and satellites detection
• planets and satellites individual
• K2-99 b
• planets and satellites
• individual
• K2-99 c
• Astrophysics - Earth and Planetary Astrophysics
• Astrophysics - Solar and Stellar Astrophysics

• All authors: 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
• Date: 2022
• Journal: Monthly Notices of the Royal Astronomical Society
• Volume: 510
• Issue: 4
• Pages: 5035 - 5049
• DOI: doi:10.1093/mnras/stab3497
• Link: https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.5035S