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Diffstat (limited to 'fg21sim/extragalactic/clusters/helper.py')
-rw-r--r-- | fg21sim/extragalactic/clusters/helper.py | 30 |
1 files changed, 30 insertions, 0 deletions
diff --git a/fg21sim/extragalactic/clusters/helper.py b/fg21sim/extragalactic/clusters/helper.py index e751bbe..f5b4f8c 100644 --- a/fg21sim/extragalactic/clusters/helper.py +++ b/fg21sim/extragalactic/clusters/helper.py @@ -26,6 +26,10 @@ References Fujita et al. 2003, ApJ, 584, 190; http://adsabs.harvard.edu/abs/2003ApJ...584..190F +.. [lokas2001] + Lokas & Mamon 2001, MNRAS, 321, 155 + http://adsabs.harvard.edu/abs/2001MNRAS.321..155L + .. [murgia2009] Murgia et al. 2009, A&A, 499, 679 http://adsabs.harvard.edu/abs/2009A%26A...499..679M @@ -446,3 +450,29 @@ def draw_halo(radius, nr=2.0, felong=None, rotation=None): # Normalized to have *mean* value of 1 image /= image.mean() return image + + +def fmass_nfw(x, c=5.0): + """ + The normalized total mass profile by integrating from the NFW + density profile. + + Parameters + ---------- + x : float + x = R/R_vir, fractional virial radius + c : float + Concentration parameter + Default: 5.0 (for clusters) + + Returns + ------- + fmass : float + The normalized total mass w.r.t. the virial mass, i.e., + fmass = M(<x*R_vir) / M_vir + + Reference: [lokas2001],Eq.(2,4,5,8) + """ + gc = 1.0 / (np.log(1+c) - c/(1+c)) + fmass = gc * (np.log(1+c*x) - c*x / (1+c*x)) + return fmass |