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Searching the literature, we found 25 stars with directly imaged planets andcandidates. We gathered photometric and spectral information for all theseobjects to derive their luminosities in a homogeneous way, taking a bolometriccorrection into account. Using theoretical evolutionary models, one can thenestimate the mass from luminosity, temperature, and age. According to our massestimates, all of them can have a mass below 25 Jup masses, so that they areconsidered as planets.

Direct Imaging of Extra-solar Planets - Homogeneous Comparison of Detected Planets and Candidates