English

Massive data compression for parameter-dependent covariance matrices

Cosmology and Nongalactic Astrophysics 2017-10-18 v2 Instrumentation and Methods for Astrophysics Methodology

Abstract

We show how the massive data compression algorithm MOPED can be used to reduce, by orders of magnitude, the number of simulated datasets that are required to estimate the covariance matrix required for the analysis of gaussian-distributed data. This is relevant when the covariance matrix cannot be calculated directly. The compression is especially valuable when the covariance matrix varies with the model parameters. In this case, it may be prohibitively expensive to run enough simulations to estimate the full covariance matrix throughout the parameter space. This compression may be particularly valuable for the next-generation of weak lensing surveys, such as proposed for Euclid and LSST, for which the number of summary data (such as band power or shear correlation estimates) is very large, 104\sim 10^4, due to the large number of tomographic redshift bins that the data will be divided into. In the pessimistic case where the covariance matrix is estimated separately for all points in an MCMC analysis, this may require an unfeasible 10910^9 simulations. We show here that MOPED can reduce this number by a factor of 1000, or a factor of 106\sim 10^6 if some regularity in the covariance matrix is assumed, reducing the number of simulations required to a manageable 10310^3, making an otherwise intractable analysis feasible.

Keywords

Cite

@article{arxiv.1707.06529,
  title  = {Massive data compression for parameter-dependent covariance matrices},
  author = {Alan Heavens and Elena Sellentin and Damien de Mijolla and Alvise Vianello},
  journal= {arXiv preprint arXiv:1707.06529},
  year   = {2017}
}

Comments

8 pages. Accepted by MNRAS

R2 v1 2026-06-22T20:52:58.716Z