SOMBI: Bayesian identification of parameter relations in unstructured cosmological data
Abstract
This work describes the implementation and application of a correlation determination method based on self organizing maps and Bayesian inference (SOMBI). SOMBI aims to automatically identify relations between different observed parameters in unstructured cosmological or astrophysical surveys by automatically identifying data clusters in highdimensional datasets via the self organizing map neural network algorithm. Parameter relations are then revealed by means of a Bayesian inference within respective identified data clusters. Specifically such relations are assumed to be parametrized as a polynomial of unknown order. The Bayesian approach results in a posterior probability distribution function for respective polynomial coefficients. To decide which polynomial order suffices to describe correlation structures in data, we include a method for model selection, the Bayesian information criterion, to the analysis. The performance of the SOMBI algorithm is tested with mock data. As illustration we also provide applications of our method to cosmological data. In particular, we present results of a correlation analysis between galaxy and active galactic nucleus (AGN) properties provided by the SDSS catalog with the cosmic largescalestructure (LSS). The results indicate that the combined galaxy and LSS dataset indeed is clustered into several subsamples of data with different average properties (for example different stellar masses or webtype classifications). The majority of data clusters appear to have a similar correlation structure between galaxy properties and the LSS. In particular we revealed a positive and linear dependency between the stellar mass, the absolute magnitude and the color of a galaxy with the corresponding cosmic density field. A remaining subset of data shows inverted correlations, which might be an artifact of nonlinear redshift distortions.
 Publication:

Astronomy and Astrophysics
 Pub Date:
 November 2016
 DOI:
 10.1051/00046361/201628393
 arXiv:
 arXiv:1602.08497
 Bibcode:
 2016A&A...595A..75F
 Keywords:

 methods: statistical;
 methods: numerical;
 largescale structure of Universe;
 methods: data analysis;
 Astrophysics  Cosmology and Nongalactic Astrophysics;
 Astrophysics  Instrumentation and Methods for Astrophysics
 EPrint:
 18 pages, 12 figures, accepted by A&