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Principled Point-source Detection in Collections of Astronomical Images

  • Authors: Dustin Lang, David W. Hogg

Dustin Lang and David W. Hogg 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

The effect of the flux prior on the decision boundaries of Bayesian SED-matched source detection. The exponential scale factor α affects the shape of the decision contours. Decision contours for three different false-positive rates are shown (10−1, 10−4, and 10−7) for two different “alpha” values (“bright”: α = 1; “faint”: α = 4). The foreground model is the three-SED model used in previous figures. The detailed shape of the decision boundary is affected by the flux prior.

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