Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements

TL;DR

SORT is a simple, efficient method that uses reference samples and stochastic ordering to improve cosmological redshift measurements, enhancing the recovery of cosmic web features and correlation functions.

Contribution

This paper introduces the Stochastic Order Redshift Technique (SORT), a novel approach leveraging stochastic ordering and reference distributions to refine redshift estimates in cosmological surveys.

Findings

SORT improves redshift accuracy and preserves cosmic web features.

It provides unbiased two-point correlation function measurements.

The method is robust and suitable for large photometric surveys.

Abstract

We present a simple, efficient and robust approach to improve cosmological redshift measurements. The method is based on the presence of a reference sample for which a precise redshift number distribution (dN/dz) can be obtained for different pencil-beam-like sub-volumes within the original survey. For each sub-volume we then impose: (i) that the redshift number distribution of the uncertain redshift measurements matches the reference dN/dz corrected by their selection functions; and (ii) the rank order in redshift of the original ensemble of uncertain measurements is preserved. The latter step is motivated by the fact that random variables drawn from Gaussian probability density functions (PDFs) of different means and arbitrarily large standard deviations satisfy stochastic ordering. We then repeat this simple algorithm for multiple arbitrary pencil-beam-like overlapping sub-volumes; in this manner, each uncertain measurement has multiple (non-independent) "recovered" redshifts which can be used to estimate a new redshift PDF. We refer to this method as the Stochastic Order Redshift Technique (SORT). We have used a state-of-the-art N-body simulation to test the performance of SORT under simple assumptions and found that it can improve the quality of cosmological redshifts in an efficient and robust manner. Particularly, SORT redshifts are able to recover the distinctive features of the 'cosmic web' and can provide unbiased measurement of the two-point correlation function on scales > 4 Mpc/h. Given its simplicity, we envision that a method like SORT can be incorporated into more sophisticated algorithms aimed to exploit the full potential of large extragalactic photometric surveys.