False color, near infrared image of the Kappa Andromedae system, by the Subaru Telescope. Almost all of the light of the host star has been removed by the dark, software-generated disk in the center. Credit: NAOJ/Subaru/J. Carson (College of Charleston)/T. Currie (University Toronto)
A "signal-to-noise ratio map" generated from the left image. The whiteness of each speckle indicates the probability that we are dealing not with an artefact ("noise"), but with the trace of a real object ("signal"). The white feature toward the upper left, representing a high signal-to-noise value, indicates the high-confidence, super-Jupiter detection. Credit: NAOJ/Subaru/J. Carson (College of Charleston)/T. Currie (University Toronto)