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Hammurabi: Simulating polarized Galactic synchrotron emissio

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kcd
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Hammurabi: Simulating polarized Galactic synchrotron emission

Postby kcd » Sun Jan 29, 2012 7:34 am

Hammurabi: Simulating polarized Galactic synchrotron emission

Abstract: The Hammurabi code is a publicly available C++ code for generating mock polarized observations of Galactic synchrotron emission with telescopes such as LOFAR, SKA, Planck, and WMAP, based on model inputs for the Galactic magnetic field (GMF), the cosmic-ray density distribution, and the thermal electron density. The Hammurabi code allows one to perform simulations of several different data sets simultaneously, providing a more reliable constraint of the magnetized ISM.

Credit: Jaffe, Tess; Waelkens, Andre; Reinecke, M.; Kitaura, F. S.; Ensslin, T. A.

Site: https://sourceforge.net/projects/hammurabicode/
http://adsabs.harvard.edu/abs/2009A%26A...495..697W

Bibcode: 2012ascl.soft01014J

ID: ascl:1201.014
Last edited by Ada Coda on Sun Apr 22, 2018 11:10 pm, edited 1 time in total.
Reason: Updated code entry.

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owlice
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Re: Hammurabi: Simulating polarized Galactic synchrotron emi

Postby owlice » Tue Jan 06, 2015 1:57 pm

The Hammurabi entry has been updated with the new code site: http://sourceforge.net/projects/hammurabicode/
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