New calculation of the atmospheric neutrino flux in a three-dimensional scheme

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Explosion mechanism, neutrino burst and gravitational wave in core-collapse supernovae (2005, background): “This is roughly correct, even though the ratio depends on a lot of factors such as neutrino energy and zenith angle of the incoming neutrino if detailed decay processes and geometric effects are taken into account [29, 139, 140].”
FERMI OBSERVATIONS OF CASSIOPEIA AND CEPHEUS: DIFFUSE GAMMA-RAY EMISSION IN THE OUTER GALAXY (2009, methodology): “More recent calculations by Mori (2009), however, report values as large as ǫN ≃ 1.75 − 2 due to different CR spectral formulae (Honda et al. 2004), different ISM abundances and the inclusion of heavier nuclei both in CRs and in the ISM.”