Redshift inference from the combination of galaxy colours and clustering in a hierarchical Bayesian model
Abstract
Powerful current and future cosmological constraints using high-precision measurements of the large-scale structure of galaxies and its weak gravitational lensing effects rely on accurate characterization of the redshift distributions of the galaxy samples using only broad-band imaging. In this paper, we present a framework for constraining both the redshift probability distributions of galaxy populations and the redshifts of their individual members. We use a hierarchical Bayesian model (HBM) which provides full posterior distributions on those redshift probability distributions, and, for the first time, we show how to combine survey photometry of single galaxies and the information contained in the galaxy clustering against a well-characterized tracer population in a robust way. One critical approximation turns the HBM into a system amenable to efficient Gibbs sampling. We show that in the absence of photometric information, this method reduces to commonly used clustering redshift estimators. Using a simple model system, we show how the incorporation of clustering information with photo-$$z$$’s tightens redshift posteriors, and can overcome biases or gaps in the coverage of a spectroscopic prior. The method enables the full propagation of redshift uncertainties into cosmological analyses, and uses all the information at hand to reduce those uncertainties and associated potential biases.
- Authors:
-
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Publication Date:
- Research Org.:
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); National Science Foundation (NSF)
- OSTI Identifier:
- 1610995
- Grant/Contract Number:
- SC0007901; AST-1311924; AST-1615555
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 483; Journal Issue: 2; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; astronomy & astrophysics; cosmology: observations; galaxy: surveys; photometric redshifts
Citation Formats
Sánchez, Carles, and Bernstein, Gary M. Redshift inference from the combination of galaxy colours and clustering in a hierarchical Bayesian model. United States: N. p., 2018.
Web. doi:10.1093/mnras/sty3222.
Sánchez, Carles, & Bernstein, Gary M. Redshift inference from the combination of galaxy colours and clustering in a hierarchical Bayesian model. United States. https://doi.org/10.1093/mnras/sty3222
Sánchez, Carles, and Bernstein, Gary M. Thu .
"Redshift inference from the combination of galaxy colours and clustering in a hierarchical Bayesian model". United States. https://doi.org/10.1093/mnras/sty3222. https://www.osti.gov/servlets/purl/1610995.
@article{osti_1610995,
title = {Redshift inference from the combination of galaxy colours and clustering in a hierarchical Bayesian model},
author = {Sánchez, Carles and Bernstein, Gary M.},
abstractNote = {Powerful current and future cosmological constraints using high-precision measurements of the large-scale structure of galaxies and its weak gravitational lensing effects rely on accurate characterization of the redshift distributions of the galaxy samples using only broad-band imaging. In this paper, we present a framework for constraining both the redshift probability distributions of galaxy populations and the redshifts of their individual members. We use a hierarchical Bayesian model (HBM) which provides full posterior distributions on those redshift probability distributions, and, for the first time, we show how to combine survey photometry of single galaxies and the information contained in the galaxy clustering against a well-characterized tracer population in a robust way. One critical approximation turns the HBM into a system amenable to efficient Gibbs sampling. We show that in the absence of photometric information, this method reduces to commonly used clustering redshift estimators. Using a simple model system, we show how the incorporation of clustering information with photo-$z$’s tightens redshift posteriors, and can overcome biases or gaps in the coverage of a spectroscopic prior. The method enables the full propagation of redshift uncertainties into cosmological analyses, and uses all the information at hand to reduce those uncertainties and associated potential biases.},
doi = {10.1093/mnras/sty3222},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 483,
place = {United States},
year = {Thu Nov 29 00:00:00 EST 2018},
month = {Thu Nov 29 00:00:00 EST 2018}
}
Web of Science
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