An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/454/2/1958/9381114/stv2036.pdf
Reference109 articles.
1. PkANN - I. Non-linear matter power spectrum interpolation through artificial neural networks
2. pkann – II. A non-linear matter power spectrum interpolator developed using artificial neural networks
3. Cosmological constraints from the CFHTLenS shear measurements using a new, accurate, and flexible way of predicting non-linear mass clustering
4. How closely do baryons follow dark matter on large scales?
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