TPZ : Photometric redshift PDFs and ancillary information by using prediction trees and random forests

TL;DR

This paper introduces TPZ, a machine learning algorithm using prediction trees and random forests to generate accurate photometric redshift PDFs, incorporating measurement errors and providing valuable ancillary information for large survey data analysis.

Contribution

The paper presents a novel, publicly available algorithm that efficiently produces photometric redshift PDFs with uncertainty estimates and additional data quality metrics, improving upon existing methods.

Findings

TPZ performs well on SDSS and DEEP2 galaxy samples.

TPZ achieves competitive results in the PHAT1 photometric redshift contest.

The algorithm provides reliable estimates of accuracy and outlier identification.

Abstract

With the growth of large photometric surveys, accurately estimating photometric redshifts, preferably as a probability density function (PDF), and fully understanding the implicit systematic uncertainties in this process has become increasingly important. In this paper, we present a new, publicly available, parallel, machine learning algorithm that generates photometric redshift PDFs by using prediction trees and random forest techniques, which we have named TPZ. This new algorithm incorporates measurement errors into the calculation while also dealing efficiently with missing values in the data. In addition, our implementation of this algorithm provides supplementary information regarding the data being analyzed, including unbiased estimates of the accuracy of the technique without resorting to a validation data set, identification of poor photometric redshift areas within the parameter space occupied by the spectroscopic training data, a quantification of the relative importance of the variables used to construct the PDF, and a robust identification of outliers. This extra information can be used to optimally target new spectroscopic observations and to improve the overall efficacy of the redshift estimation. We have tested TPZ on galaxy samples drawn from the SDSS main galaxy sample and from the DEEP2 survey, obtaining excellent results in each case. We also have tested our implementation by participating in the PHAT1 project, which is a blind photometric redshift contest, finding that TPZ performs comparable to if not better than other empirical photometric redshift algorithms. Finally, we discuss the various parameters that control the operation of TPZ, the specific limitations of this approach and an application of photometric redshift PDFs.