| Commit message (Collapse) | Author | Age | Files | Lines |
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* GalacticSNRs_Green2014.csv
* Halpha_fwhm06_ns1024.fits.xz
* SFD_i100_ns1024.fits.xz
* haslam408_dsds_Remazeilles2014_ns512.fits.xz
* synchrotron_specind2_ns512.fits.xz
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Adopt the same beta-model for the gas density profile to calculate the
gas/baryon mass within the turbulence region (<R_turb).
Meanwhile, change the '_velocity_turb()` method to a property without
depending on the time, to further simplify the model a bit.
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This function calculates the stripping radius of the sub-cluster when it
falling through the main cluster.
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Also update the data manifest and the user guide page.
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