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  Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection

Oddo, A., Sefusatti, E., Porciani, C., Monaco, P., & Sánchez, A. G. (2020). Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection. Journal of Cosmology and Astroparticle Physics, 2020(3): 056. doi:10.1088/1475-7516/2020/03/056.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0006-98A7-2 Version Permalink: http://hdl.handle.net/21.11116/0000-0006-98A8-1
Genre: Journal Article

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 Creators:
Oddo, Andrea, Author
Sefusatti, Emiliano, Author
Porciani, Cristiano, Author
Monaco, Pierluigi, Author
Sánchez, Ariel G.1, Author              
Affiliations:
1Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              

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 Abstract: The forthcoming generation of galaxy redshift surveys will sample the large-scale structure of the Universe over unprecedented volumes with high-density tracers. This advancement will make robust measurements of three-point clustering statistics possible. In preparation for this improvement, we investigate how several methodological choices can influence inferences based on the bispectrum about galaxy bias and shot noise. We first measure the real-space bispectrum of dark-matter haloes extracted from 298 N-body simulations covering a volume of approximately 1000 Gpc3. We then fit a series of theoretical models based on tree-level perturbation theory to the numerical data. To achieve this, we estimate the covariance matrix of the measurement errors by using 10,000 mock catalogues generated with the PINOCCHIO code. We study how the model constraints are influenced by the binning strategy for the bispectrum configurations and by the form of the likelihood function. We also use Bayesian model-selection techniques to single out the optimal theoretical description of our data. We find that a three-parameter bias model combined with Poissonian shot noise is necessary to model the halo bispectrum up to scales of kmax≲0.08 Mpc-1, although fitting formulae that relate the bias parameters can be helpful to reduce the freedom of the model without compromising accuracy. Our data clearly disfavour local Eulerian and local Lagrangian bias models and do not require corrections to Poissonian shot noise. We anticipate that model-selection diagnostics will be particularly useful to extend the analysis to smaller scales as, in this case, the number of model parameters will grow significantly large.

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Language(s): eng - English
 Dates: 2020-03-27
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Method: Peer
 Identifiers: DOI: 10.1088/1475-7516/2020/03/056
Other: LOCALID: 3239345
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Title: Journal of Cosmology and Astroparticle Physics
  Abbreviation : J. Cosmol. Astropart. Phys.
  Abbreviation : JCAP
Source Genre: Journal
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Pages: - Volume / Issue: 2020 (3) Sequence Number: 056 Start / End Page: - Identifier: ISSN: 1475-7516