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Fig. 3


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Measured contrast of each companion at the measured separations with stacked 5σ contrast curves corresponding to measured on-sky performance from VLT/SPHERE data for IRDIS H2 bands. The detection probability scale is shown on the right. The darker color corresponds to a lower likelihood of detectability with imaging with VLT/SPHERE IRDIS H2 band, and the lighter colors correspond to a higher likelihood of detectability at a given separation and contrast ratio. The astrometry and photometry for HD 157338 and HD 195010 are each shown as an average of the two 2021 SPHERE H2 band data points.

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