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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 13.

True and observed redshift histograms for the mock galaxy sample of Section 5.3. As in Figure 7, the bin edges are shown using the vertical dashed lines. We see that, as in Figure 7, the photo-z uncertainties lead to a smearing of the redshift information, while the truncation of the edge bins makes the N(z) biased near the outermost edges.

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