Precise masses for the transiting planetary system HD 106315 with HARPS
Context. The multi-planetary system HD 106315 was recently found in K2 data. The planets have periods of P b ∼ 9.55 and P c ∼ 21.06 days, and radii of r b = 2.44 ± 0.17 R ⊕ and r c = 4.35 ± 0.23 R ⊕ . The brightness of the host star (V = 9.0 mag) makes it an excellent target for transmission spectro...
Guardado en:
Autores principales: | Barros, S.C.C., Gosselin, H., Lillo-Box, J., Bayliss, D., Delgado Mena, E., Brugger, B., Santerne, A., Armstrong, D.J., Adibekyan, V., Armstrong, J.D., Barrado, D., Bento, J., Boisse, I., Bonomo, A.S., Bouchy, F., Brown, D.J.A., Cochran, W.D., Collier Cameron, A., Deleuil, M., Demangeon, O., Díaz, R.F., Doyle, A., Dumusque, X., Ehrenreich, D., Espinoza, N., Faedi, F., Faria, J.P., Figueira, P., Foxell, E., Hébrard, G., Hojjatpanah, S., Jackman, J., Lendl, M., Ligi, R., Lovis, C., Melo, C., Mousis, O., Neal, J.J., Osborn, H.P., Pollacco, D., Santos, N.C., Sefako, R., Shporer, A., Sousa, S.G., Triaud, A.H.M.J., Udry, S., Vigan, A., Wyttenbach, A. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v608_n_p_Barros |
Aporte de: |
Ejemplares similares
-
Precise masses for the transiting planetary system HD 106315 with HARPS
Publicado: (2017) -
Activity induced variation in spin-orbit angles as derived from Rossiter-McLaughlin measurements
por: Oshagh, M., et al. -
Activity induced variation in spin-orbit angles as derived from Rossiter-McLaughlin measurements
Publicado: (2018) -
Exoplanetas en torno de estrellas pequeñas y la búsqueda de vida fuera del Sistema Solar
por: Díaz, Rodrigo F.
Publicado: (2019) -
Automated code for the selection of targets to be observed with the SAINT-EX telescope
por: Petrucci, Romina, et al.
Publicado: (2022)