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Matched Filtering for the Canadian Hydrogen Observatory and Radio-transient Detector Galaxy Search

  • Authors: Hans S. Hopkins, Dustin Lang, Kendrick Smith, Kristine Spekkens, Simon Foreman, Akanksha Bij

Hans S. Hopkins et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 12.

An illustration of the 1σ, 3σ, and 5σ contours of the two-dimensional PDF of the matched-filter value of a source and an alias with important regions highlighted. The source has 7σ in brightness, and the alias’s correlation coefficient is 0.7. A detection threshold is shown at 5σ, and the region above the M(u0) = M(u1) line is the case where the alias is brighter than the true source (i.e., the alias mislocalization region). A higher correlation coefficient shifts the center of the PDF closer to this line, but it also makes the contours thinner. For each detected galaxy, a value is drawn from a similar PDF, and unlucky draws will cause the final catalog to lack completeness or reliability.

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