Prompt neutrino fluxes:
theoretical predictions

• GMS 2015:
• table of ($\nu_\mu$ + $\bar{\nu}_\mu$) flux predictions for the five different cosmic ray spectra
  of Fig. 1 of our paper. For each flux the upper and lower limit of theoretical
  QCD uncertainties are provided, together with the central flux value.

When using these predictions please quote Ref.
M.V. Garzelli, S. Moch, G. Sigl, JHEP 10 (2015) 115 , [arXiv:1507.01570] .


• PROSA 2016:
• table of ($\nu_\mu$ + $\bar{\nu}_\mu$) flux predictions for the five different cosmic ray spectra
  of Fig. 2 and 3 of our paper. For each flux the upper and lower limit of theoretical
  QCD uncertainties are provided, together with the central flux value.

When using these predictions please quote Ref.
M.V. Garzelli, et al., JHEP 05 (2017) 004 , [arXiv:1611.03815] .


• GM-VFNS 2017:
• table of ($\nu_\mu$ + $\bar{\nu}_\mu$) flux predictions for the six different cosmic ray spectra
  of Fig. 8 of our paper. For each flux the upper and lower limit of theoretical
  QCD uncertainties are provided, together with the central flux value.

When using these predictions please quote Ref.
M. Benzke, M.V. Garzelli, B. Kniehl, G. Kramer, S. Moch, G. Sigl,
JHEP 1712 (2017) 021 , [arXiv:1705.10386] .

Maria V. Garzelli / Sven-Olav Moch / Guenter Sigl
University of Hamburg,  II Institute for Theoretical Physics,
Luruper Chaussee 149,  22761 Hamburg,  Germany
Tel. + 49 (0)40 89982260    Fax + 49 (0)40 89982267
e-mail: garzelli@mail.desy.de, sven-olaf.moch@desy.de, guenter.sigl@desy.de