TY  - GEN 
AU  - Balsalobre-Ruza, O.
AU  - Lillo-Box, J.
AU  - Silva, A.M.
AU  - Grouffal, S.
AU  - Aceituno, J.
AU  - Castro-González, A.
AU  - Cifuentes, C.
AU  - Standing, M.R.
AU  - Faria, J.P.
AU  - Figueira, P.
AU  - Santerne, A.
AU  - Gómez Marfil, Emilio
AU  - Abreu, A.
AU  - Aguichine, A.
AU  - González-Ramírez, L.
AU  - Morales, J.C.
AU  - Santos, N.
AU  - Huelamo, N.
AU  - Delgado Mena, E.
AU  - Barrado, D.
AU  - Adibekyan, V.
AU  - Barros, S.C.C.
AU  - Berihuete Macías, Ángel
AU  - Morales-Calderón, M.
AU  - Nagel, E.
A4  - Estadística e Investigación Operativa
A4  - Física Aplicada
PY  - 2025
SN  - 1432-0746
SN  - 0004-6361
UR  - http://hdl.handle.net/10498/36389
AB  - Context. K-dwarf stars are promising targets in the exploration of potentially habitable planets. Their properties, falling between G and M dwarfs, provide an optimal trade-off between the prospect of habitability and ease of detection. The KOBE...
LA  - eng
PB  - EDP Sciences
KW  - Planets and satellites
KW  - detection
KW  - Stars: late-type
KW  - Surveys
KW  - Techniques
KW  - radial velocities
TI  - KOBE-1: The first planetary system from the KOBE survey: Two planets likely residing in the sub-Neptune mass regime around a late K-dwarf
DO  - 10.1051/0004-6361/202452631
ER  -