The GAPS programme at TNG. LII. Spot modelling of V1298 Tau using the SpotCCF tool
Context. The intrinsic variability due to the magnetic activity of young active stars is one of the main challenges in detecting and characterising exoplanets. The stellar activity is responsible for jitter effects observed both in photometric and spectroscopic observations that can impact our planetary detection sensitivity. Aims: We present a
Di Maio, C. et al.
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2024