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GEOMAX: beyond linear compression for three-point galaxy clustering statistics

Gualdi, D; Gil-Marín, H; Manera, M; Joachimi, B; Lahav, O; (2020) GEOMAX: beyond linear compression for three-point galaxy clustering statistics. Monthly Notices of the Royal Astronomical Society , 497 (1) pp. 776-792. 10.1093/mnras/staa1941. Green open access

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Abstract

We present the GEOMAX algorithm and its PYTHON implementation for a two-step compression of bispectrum measurements. The first step groups bispectra by the geometric properties of their arguments; the second step then maximizes the Fisher information with respect to a chosen set of model parameters in each group. The algorithm only requires the derivatives of the data vector with respect to the parameters and a small number of mock data, producing an effective, non-linear compression. By applying GEOMAX to bispectrum monopole measurements from BOSS DR12 CMASS redshift-space galaxy clustering data, we reduce the 68 per cent credible intervals for the inferred parameters (b1, b2, f, σ8) by 50.4, 56.1, 33.2, and 38.3 per cent with respect to standard MCMC on the full data vector. We run the analysis and comparison between compression methods over 100 galaxy mocks to test the statistical significance of the improvements. On average, GEOMAX performs ∼15 per cent better than geometrical or maximal linear compression alone and is consistent with being lossless. Given its flexibility, the GEOMAX approach has the potential to optimally exploit three-point statistics of various cosmological probes like weak lensing or line-intensity maps from current and future cosmological data sets such as DESI, Euclid, PFS, and SKA.

Type: Article
Title: GEOMAX: beyond linear compression for three-point galaxy clustering statistics
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/staa1941
Publisher version: https://doi.org/10.1093/mnras/staa1941
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: methods: analytical, cosmological parameters, large-scale structure of Universe
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10104850
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