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Angular Correlation Function Estimators Accounting for Contamination from Probabilistic Distance Measurements

  • Authors: Humna Awan and Eric Gawiser

2020 The Astrophysical Journal 890 78.

  • Provider: AAS Journals

Caption: Figure 4.

Distribution of the classification probabilities to be in bin 1 (upper panel) or bin 2 (lower panel) for the toy galaxy sample of Section 5.1. As introduced in Section 3, ﹩{q}_{\alpha \beta }﹩ is the probability of the observed Type-α galaxy to be a true Type-β galaxy. We see that given the photo-z uncertainties, the probability to be in a given target tomographic bin has a broad range. Note that the two panels are mirror images of one another, as dictated by the identity in Equation (7).

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