Browsing Institutt for geofag by Author "Farrington, C.D."
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Caballero, J.A.; González-Álvarez, E.; Brady, M.; Trifonov, T.; Ellis, T.G.; Dorn, C.; Cifuentes, C.; Molaverdikhani, K.; Bean, J.L.; Boyajian, T.; Rodríguez, E.; Sanz-Forcada, J.; Zapatero Osorio, Osorio; Abia, C.; Amado, P.J.; Anugu, N.; Béjar, V.J.S.; Davies, C.L.; Dreizler, S.; Dubois, F.; Ennis, J.; Espinoza, N.; Farrington, C.D.; López, A. García; Gardner, T.; Hatzes, A.P.; Henning, Th.; Herrero, E.; Herrero-Cisneros, E.; Kaminski, A.; Kasper, D.; Klement, R.; Kraus, S.; Labdon, A.; Lanthermann, C.; Le Bouquin, Bouquin; González, M. J. Lópej; Luque, R.; Mann, A.W.; Marfil, E.; Monnier, J.D.; Montes, D.; Morales, J.C.; Pallé, E.; Pedraz, S.; Quirrenbach, A.; Reffert, S.; Reiners, A.; Ribas, I.; Rodríguez-López, C.; Schaefer, G.; Schweitzer, A.; Seifahrt, A.; Setterholm, B.R.; Shan, Yutong; Shulyak, D.; Solano, E.; Sreenivas, K.R.; Stefánsson, G.; Stürmer, J.; Tabernero, H.M.; Tal-Or, L.; Ten Brummelaar, Brummelaar; Vanaverbeke, S.; Von Braun, Braun; Youngblood, A.; Zechmeister, M. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2022)Context . The Gl 486 system consists of a very nearby, relatively bright, weakly active M3.5 V star at just 8 pc with a warm transiting rocky planet of about 1.3 R ⊕ and 3.0 M ⊕ . It is ideal for both transmission and ...