TY  - JOUR 
AU  - Zechmeister, M.
AU  - Suárez Yanes, Juan Carlos
PY  - 2019
UR  - http://hdl.handle.net/10481/56129
AB  - Context.Teegarden’s Star is the brightest and one of the nearest ultra-cool dwarfs in the solar neighbourhood. For its late spectral type (M7.0 V),the star shows relatively little activity and is a prime target for near-infrared radial velocity...
LA  - eng
PB  - EDP Sciences
KW  - Methods: data analysis
KW  - Planetary systems
KW  - Stars: late-type
KW  - Stars: individual: Teegarden’s Star
TI  - The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden’s Star
DO  - 10.1051/0004-6361/201935460
ER  -