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The-wiZZ: Clustering redshift estimation for everyone

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arxiv 1609.09085 v2 pith:RQQDYH6C submitted 2016-09-28 astro-ph.CO astro-ph.GAastro-ph.IM

classification astro-ph.COastro-ph.GAastro-ph.IM
keywords redshiftclusteringredshiftssurveythe-wizzestimationsamplegalaxies
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We present The-wiZZ, an open source and user-friendly software for estimating the redshift distributions of photometric galaxies with unknown redshifts by spatially cross-correlating them against a reference sample with known redshifts. The main benefit of The-wiZZ is in separating the angular pair finding and correlation estimation from the computation of the output clustering redshifts allowing anyone to create a clustering redshift for their sample without the intervention of an "expert". It allows the end user of a given survey to select any sub-sample of photometric galaxies with unknown redshifts, match this sample's catalog indices into a value-added data file, and produce a clustering redshift estimation for this sample in a fraction of the time it would take to run all the angular correlations needed to produce a clustering redshift. We show results with this software using photometric data from the Kilo-Degree Survey (KiDS) and spectroscopic redshifts from the Galaxy and Mass Assembly (GAMA) survey and the Sloan Digital Sky Survey (SDSS). The results we present for KiDS are consistent with the redshift distributions used in a recent cosmic shear analysis from the survey. We also present results using a hybrid machine learning-clustering redshift analysis that enables the estimation of clustering redshifts for individual galaxies. The-wiZZ can be downloaded at http://github.com/morriscb/The-wiZZ/.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Tomographer: End-to-end Redshift Distribution Estimation for Source Catalogs and Intensity Maps

    astro-ph.CO 2026-08 conditional novelty 6.0 of 10

    Tomographer recovers bias-weighted redshift distributions b(z)dN/dz or b(z)dI/dz from source catalogs or intensity maps in minutes, using precomputed activation maps instead of user-side pair counting.

  2. Cosmology and Source Redshift Distributions from Combining Radio Weak Lensing with CMB Lensing

    astro-ph.CO 2024-12 conditional novelty 6.0 of 10

    Cross-correlating radio cosmic shear with CMB lensing could calibrate radio source redshift distributions to 1-10% and tighten neutrino mass forecasts by ~20-24% over an Euclid-like survey.

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