The CARMENES search for exoplanets around M dwarfs: Understanding the wavelength dependence of radial velocity measurements
Context. Current exoplanet surveys are focused on detecting small exoplanets orbiting in the liquid-water habitable zones of their host stars. Despite recent significant advancements in instrumentation, the main limitation in detecting these exoplanets is the intrinsic variability of the host star itself. Aims. Our aim is to investigate the
Jeffers, S. V. et al.
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2025