SHINE presents homogeneous stellar properties and a vetted subsample of 333 young single stars from 460 targets observed with SPHERE direct imaging between 2015 and 2023.
is probable very wide companion (Majidi et al. 2020). HIP 76395.The star is classified as a close, equal-mass binary (ρ=0.2
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The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization
SHINE presents homogeneous stellar properties and a vetted subsample of 333 young single stars from 460 targets observed with SPHERE direct imaging between 2015 and 2023.