Fuhrmeister, B.; Czesla, S.; Perdelwitz, V.; Nagel, E.; Schmitt, J. H. M. M.; Jeffers, S. V.; Caballero, J. A.; Zechmeister, M.; Montes, D.; Reiners, A.et al.; López-Gallifa, Á.; Ribas, I.; Quirrenbach, A.; Amado, P. J.; Galadí-Enríquez, D.; Béjar, V. J. S.; Danielski, C.; Hatzes, A. P.; Kaminski, A.; Kürster, M.; Morales, J. C.; Zapatero Osorio, M. R.: The CARMENES search for exoplanets around M dwarfs. Variability on long timescales as seen in chromospheric indicators. Astronomy and Astrophysics 670, p. A71 (2023)
Fuhrmeister, B.; Czesla, S.; Nagel, E.; Reiners, A.; Schmitt, J. H. M. M.; Jeffers, S. V.; Caballero, J. A.; Shulyak, D.; Johnson, E. N.; Zechmeister, M.et al.; Montes, D.; López-Gallifa, Á.; Ribas, I.; Quirrenbach, A.; Amado, P. J.; Galadí-Enríquez, D.; Hatzes, A. P.; Kürster, M.; Danielski, C.; Béjar, V. J. S.; Kaminski, A.; Morales, J. C.; Zapatero Osorio, M. R.: The CARMENES search for exoplanets around M dwarfs. Diagnostic capabilities of strong K I lines for photosphere and chromosphere. Astronomy and Astrophysics 657, p. A125 (2022)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.