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Lucas-Kuhnxzackli
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Update profiles_rsz.jl
Updates to T scaling function to include results from different simulations
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src/profiles_rsz.jl

Lines changed: 27 additions & 2 deletions
Original file line numberDiff line numberDiff line change
@@ -46,13 +46,38 @@ function T_vir_calc(𝕡,M,z::T) where T
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return T_vir
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end
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49-
function rSZ(𝕡, M_200, z, r, showT=true)
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function T_mass_calc(𝕡,M,z::T; scale_type="Ty", sim_type="combination") where T
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"""
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Calculates the temperature for a given halo using https://arxiv.org/pdf/2207.05834.pdf.
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"""
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E_z = 𝕡.cosmo.Ω_m*(1 + z)^3 + 𝕡.cosmo.Ω_Λ
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par_dict_scale = Dict([("Ty",[1.426,0.566,0.024]),("Tm",[1.207,0.589,0.003]),("Tsl",[1.196,0.641,-0.048])])
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par_dict_sim = Dict([("combination",[1.426,0.566,0.024]),("bahamas",[2.690,0.323,0.023]),("the300",[2.294,0.350,0.013]),("magneticum",[2.789,0.379,0.030]),("tng",[2.154,0.365,0.032])])
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if scale_type=="Ty"
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params = par_dict_sim[sim_type]
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else
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params = par_dict_scale[scale_type]
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end
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T_e = E_z^(2/3) * params[1] * (M/(10^14 *M_sun))^(params[2] + params[3] * log10(M/(10^14 * M_sun))) * u"keV"
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return T_e
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end
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function rSZ(𝕡, M_200, z, r; T_scale="virial", sim_type="combination", showT=true)
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"""
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Calculates the integrated relativistic compton-y signal along the line of sight.
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"""
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#X = (constants.ħ*ω)/(constants.k_B*T_cmb) # omega is standard frequency in Hz
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X = 𝕡.X
55-
T_e = T_vir_calc(𝕡, M_200, z)
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if T_scale=="virial"
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T_e = T_vir_calc(𝕡, M_200, z)
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elseif typeof(T_scale)==String
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T_e = uconvert(u"K",(T_mass_calc(𝕡, M_200, z, scale_type=T_scale, sim_type=sim_type)/constants.k_B))
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else
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T_e = T_scale
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end
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θ_e = (constants.k_B*T_e)/(constants.m_e*constants.c_0^2)
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ω = (X*constants.k_B*T_cmb)/constants.h
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