# Phenotypic redshifts with self-organizing maps: A novel method to   characterize redshift distributions of source galaxies for weak lensing

**Authors:** R. Buchs, C. Davis, D. Gruen, J. DeRose, A. Alarcon, G. M. Bernstein,, C. S\'anchez, J. Myles, A. Roodman, S. Allen, A. Amon, A. Choi, D. C., Masters, R. Miquel, M. A. Troxel, R. H. Wechsler, T. M. C. Abbott, J. Annis,, S. Avila, K. Bechtol, S. L. Bridle, D. Brooks, E. Buckley-Geer, D. L. Burke,, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, R., Cawthon, C. B. D'Andrea, L. N. da Costa, J. De Vicente, S. Desai, H. T., Diehl, P. Doel, A. Drlica-Wagner, T. F. Eifler, A. E. Evrard, B. Flaugher, P., Fosalba, J. Frieman, J. Garc\'ia-Bellido, E. Gaztanaga, R. A. Gruend, J., Gschwend, G. Gutierrez, W. G. Hartley, D. L. Hollowood, K. Honscheid, D. J., James, K. Kuehn, N. Kuropatkin, M. Lima, H. Lin, M. A. G. Maia, M. March, J., L. Marshall, P. Melchior, F. Menanteau, R. L. C. Ogando, A. A. Plazas, E. S., Rykoff, E. Sanchez, V. Scarpine, S. Serrano, I. Sevilla-Noarbe, M. Smith, M., Soares-Santos, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarle, D., Thomas, V. Vikram

arXiv: 1901.05005 · 2019-08-14

## TL;DR

This paper introduces a new phenotypic redshift method using self-organizing maps to improve redshift distribution estimates for weak lensing surveys, reducing uncertainties significantly.

## Contribution

The novel approach combines wide-field, few-filter data with deep field catalogs using self-organizing maps to enhance redshift calibration accuracy.

## Key findings

- Achieved a redshift uncertainty of 0.007 in simulated DES data
- Reduced redshift calibration error by 60% compared to previous analysis
- Method applicable to other large photometric surveys

## Abstract

Wide-field imaging surveys such as the Dark Energy Survey (DES) rely on coarse measurements of spectral energy distributions in a few filters to estimate the redshift distribution of source galaxies. In this regime, sample variance, shot noise, and selection effects limit the attainable accuracy of redshift calibration and thus of cosmological constraints. We present a new method to combine wide-field, few-filter measurements with catalogs from deep fields with additional filters and sufficiently low photometric noise to break degeneracies in photometric redshifts. The multi-band deep field is used as an intermediary between wide-field observations and accurate redshifts, greatly reducing sample variance, shot noise, and selection effects. Our implementation of the method uses self-organizing maps to group galaxies into phenotypes based on their observed fluxes, and is tested using a mock DES catalog created from N-body simulations. It yields a typical uncertainty on the mean redshift in each of five tomographic bins for an idealized simulation of the DES Year 3 weak-lensing tomographic analysis of $\sigma_{\Delta z} = 0.007$, which is a 60% improvement compared to the Year 1 analysis. Although the implementation of the method is tailored to DES, its formalism can be applied to other large photometric surveys with a similar observing strategy.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/1901.05005/full.md

## References

76 references — full list in the complete paper: https://tomesphere.com/paper/1901.05005/full.md

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Source: https://tomesphere.com/paper/1901.05005