Calibrating Redshift Distributions beyond Spectroscopic Limits with Cross‐Correlations
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We describe a new method that can measure the true redshift distribution of any set of objects that are studied only photometrically. Measuring the angular cross-correlation between objects in the photometric sample with objects in some spectroscopic sample as a function of the spectroscopic z , along with other, standard correlation measurements, provides sufficient information to reconstruct the redshift distribution of the photometric sample. The spectroscopic sample need not resemble the photometric sample in galaxy properties, but must fall within its sky coverage. We test this hybrid, photometric-spectroscopic cross-correlation technique with Monte Carlo simulations based on realistic error estimates (including sample variance). The rms errors in recovering both the mean redshift and σ of the redshift distribution for a single photometric redshift bin with true distribution given by a Gaussian are 1.4 × 10 −3 (σ z /0.1)(Σ p /10) −0.3 (d N s / dz /25,000) −1/2 , where σ z is the true Gaussian σ , Σ p is the surface density of the photometric sample in galaxies arcmin −2 , and dN s / dz is the number of galaxies with a spectroscopic redshift per unit z . We test the impact of non-Gaussian redshift outliers and of systematic errors due to unaccounted-for bias evolution, errors in measuring autocorrelations, photometric zero-point variations, or mistaken cosmological assumptions, and find that none will dominate measurement uncertainties in reasonable scenarios. The true redshift distributions of even arbitrarily faint photometric samples may be determined to the precision required by proposed dark energy experiments (Δ⟨ z ⟩ ≲ 3 × 10 −3 at z ∼ 1) with this method.
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Photometric redshift calibration can be further improved by cross-correlating the photometric sample with redshift surveys of galaxies and quasars in the same fields.
“It will be possible to further improve photometric redshift calibration by crosscorrelating the photometric sample with redshift surveys of galaxies and quasars in the same fi elds ( Newman 2008; Matthews & Newman 2010; Ménard et al. 2013; Davis et al. 2017 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Newman 2008
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Dark Energy Survey Year 1 Results: redshift distributions of the weak-lensing source galaxies
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Target Selection and Validation of DESI Emission Line Galaxies
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PHOTOMETRIC REDSHIFT WITH BAYESIAN PRIORS ON PHYSICAL PROPERTIES OF GALAXIES
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ULTRA-LARGE-SCALE COSMOLOGY IN NEXT-GENERATION EXPERIMENTS WITH SINGLE TRACERS
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ArborZ: PHOTOMETRIC REDSHIFTS USING BOOSTED DECISION TREES
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WISE x Supercosmos photometric redshift catalog: 20 million galaxies over 3 pi steradians
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The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Analysis and Data Release 2
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Parameter constraints from cross-correlation of CMB lensing with galaxy clustering
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COMPREHENSIVE TWO-POINT ANALYSES OF WEAK GRAVITATIONAL LENSING SURVEYS
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Photometric redshift calibration with self-organising maps
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Photometric Redshifts for Next-Generation Surveys
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Spectroscopic needs for imaging dark energy experiments
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RCSLenS: The Red Cluster Sequence Lensing Survey
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The LSST DESC DC2 Simulated Sky Survey
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RECONSTRUCTING REDSHIFT DISTRIBUTIONS WITH CROSS-CORRELATIONS: TESTS AND AN OPTIMIZED RECIPE
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Self-citationunWISE tomography of Planck CMB lensing
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Cosmology with the Large Synoptic Survey Telescope: an overview
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the-wizz: clustering redshift estimation for everyone
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Reconstructing large-scale structure with neutral hydrogen surveys
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Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release
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Incompleteness Matters Not: Inference of H0 from Binary Black Hole–Galaxy Cross-correlations
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Clustering-based redshift estimation: comparison to spectroscopic redshifts
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UnWISE tomography of Planck CMB lensing
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KiDS-1000: Cosmic shear with enhanced redshift calibration
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- Authors
- Newman, J. A.
- Affiliations
- University of Pittsburgh (US)
- Corresponding author
- Newman, Jeffrey A.
- ORCID
- Newman, Jeffrey A.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2008-09
- Volume
- 684
- Issue
- 1
- Pages
- 88-101
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2048401217
- Cited by
- 285
- References
- 54
- Citations by year
- 2026: 12 · 2025: 15 · 2024: 14 · 2023: 20 · 2022: 18 · 2021: 27 · 2020: 28 · 2019: 21 · 2018: 20 · 2017: 15 · 2016: 25 · 2015: 14 · 2014: 13 · 2013: 8 · 2012: 11
- FWCI
- 4.67
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration (NAS 526555)
- Space Telescope Science Institute (NAS5- 26555, 26555)
- Lawrence Berkeley National Laboratory
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Keywords
- photometric redshifts, angular cross-correlation, spectroscopic redshifts, sample variance, Dark Energy Survey, Monte Carlo simulation
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