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Cited article:

Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys

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Monthly Notices of the Royal Astronomical Society 503 (2) 1999 (2021)
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Non-Gaussianity in the weak lensing correlation function likelihood – implications for cosmological parameter biases

Chien-Hao Lin, Joachim Harnois-Déraps, Tim Eifler, et al.
Monthly Notices of the Royal Astronomical Society 499 (2) 2977 (2020)
https://doi.org/10.1093/mnras/staa2948

Cosmological inference from galaxy-clustering power spectrum: Gaussianization and covariance decomposition

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Monthly Notices of the Royal Astronomical Society 486 (1) 951 (2019)
https://doi.org/10.1093/mnras/stz829

Modelling bivariate astronomical data with multiple components and non-linear relationships

C. Koen and A. Bere
Monthly Notices of the Royal Astronomical Society 471 (3) 2771 (2017)
https://doi.org/10.1093/mnras/stx1740

CFHTLenS: a Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics

P. Simon, E. Semboloni, L. van Waerbeke, et al.
Monthly Notices of the Royal Astronomical Society 449 (2) 1505 (2015)
https://doi.org/10.1093/mnras/stv339