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J/A+A/534/A54       GALPROP programme                        (Strong+, 2011)

The interstellar cosmic-ray electron spectrum from synchrotron radiation and direct measurements. Strong A.W., Orlando E., Jaffe T.R. <Astron. Astrophys. 534, A54 (2011)> =2011A&A...534A..54S
ADC_Keywords: Models ; Gamma rays Keywords: radio continuum: galaxies - ISM: magnetic fields - gamma rays: ISM - Galaxy: structure - cosmic rays Abstract: We exploit synchrotron radiation to constrain the low-energy interstellar electron spectrum, using various radio surveys and connecting with electron data from Fermi-LAT and other experiments. The GALPROP programme for cosmic-ray propagation, gamma-ray and synchrotron radiation is used. Secondary electrons and positrons are included. Propagation models based on cosmic-ray and gamma-ray data are tested against synchrotron data from 22MHz to 94GHz. Description: This document (galprop_v54.pdf) provides a description of Version 54 of the GALPROP cosmic ray propagation code. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file galprop_v54.pdf 512 1147 GALPROP Version 54: Explanatory Supplement
Acknowledgements: Andrew Strong, aws(at)
(End) Patricia Vannier [CDS] 30-Sep-2011
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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