A hot sub-Neptune in the desert and a temperate super-Earth around faint M dwarfs. Color validation of TOI-4479b and TOI-2081b

Author(s):
Esparza-Borges, E.; Parviainen, H.; Murgas, F.; Pallé, E.; Maas, A.; Morello, G.; Zapatero-Osorio, M.R.; Barkaoui, K.; Narita, N.; Fukui, A.; Casasayas Barris, N.; Oshagh, M.; Crouzet, N.M.; Galán, D.; Fernández, G.E.; Kagetani, T.; Kawauchi, K.; Kodama, T.; Korth, J.; Kusakabe, N.; Laza-Ramos, A.; Luque, R.; Livingston, J.; Madrigal-Aguado, A.; Mori, M.; Orell-Miquel, J.; Puig-Subirà, M.; Stangret, M.; Terada, Y.; Watanabe, N.; Zou, Y.; Baliga Savel, A.; Belinski, A.A.; Collins, K.; Dressing, C.D.; Giacalone, S.; Gill, H.; Goliguzova, M.V.; Ikoma, M.; Jenkins, J.M.; Tamura, M.; Twicken, J.D.; Ricker, G.R.; Schwarz, R.P.; Seager, S.; Shporer, A.; Vanderspek, R.; Winn, J.
Published
2022
Publication type
Article / Letter to editor
Planets and satellites - individual - TOI-4479bPlanets and satellites - individual - TOI-2081bMethods - observationalTechniques - photometricPlanets and satellites - generalPlanets and satellites - detectionAstrophysics - earth and planetary astrophysicsAstrophysics - solar and stellar astrophysics
Date issued
2022
Language
English
Is part of
Astronomy & Astrophysics (2022), A10
hdl
1887/3515357
doi
10.1051/0004-6361/202243731
URL
https://ui.adsabs.harvard.edu/abs/2022A&A...666A..10E