renamed magdziarz sed program

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caes 2016-06-01 03:38:17 -04:00
parent c05603cc94
commit a6bea59974

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@ -0,0 +1,108 @@
#parents, babies = (1, 1)
#while babies < 100:
# #print 'This generation has {0} babies'.format(babies)
# print('This generation has',babies,'babies.')
# parents, babies = (babies, parents + babies)
import math
PI=3.14159265358979323846;
PLANCK_CONST=4.135668e-15; # in eV * s
BOLTZMANN_CONST=0.00008617332385; # in eV / K
RYDBERG_CONST=1.0973731568539e7; # in 1 / m
RYDBERG_UNIT_EV=13.60569252; # in eV
RYDBERG_UNIT_ANGSTROM=1e10/RYDBERG_CONST; # in A
CONT_MIN_ENERGY_keV = 1e-5; # eV
CONT_MAX_ENERGY_keV = 1e2; # eV
CONT_MIN_X = math.log10(CONT_MIN_ENERGY_keV);
CONT_MAX_X = math.log10(CONT_MAX_ENERGY_keV);
CONT_WIDTH_X = CONT_MAX_X - CONT_MIN_X;
CONT_MIN_VAL = 1e-35;
""" Cloudy's continuum domain, for reference, version 13.3 """
CLOUDY_EMM = 1.001e-8; # in Rydberg
CLOUDY_EGAMRY = 7.354e6; # in Rydberg
CLOUDY_MIN_EV = CLOUDY_EMM*RYDBERG_UNIT_EV;
CLOUDY_MAX_EV = CLOUDY_EGAMRY*RYDBERG_UNIT_EV;
IN_EV_2500A = 12398.41929/2500;
""" Curve Parameters from MNRAS 301 Mdagziarz 1998 """
α_HC = 0.86
# Soft Excess
α_SE = 1.1 # Quoted consistent with Korista 1995 and Marshall 1997
kT_SE = .56
# Comtonization fitted to ROSAT data
# ξ =
# OSSE data fit
α_HC = 0.86
R = 0.96
E_cutoff_HC = 120 # keV, phase 1
F_HC = .38 # keV cm⁻² s⁻¹
# E_cutoff_HC = 118 # keV, phase 3
# F_HC = .61 # keV cm⁻² s⁻¹
def hν_at(i,n):
""" returns hν coordinate of bin i out of n """
relative_coord = i/n
x_coord = relative_coord*CONT_WIDTH_X + CONT_MIN_X;
return math.pow(10,x_coord);
def histogram_table(n):
output = []
# max=0,min=1
indices = range(n)
for i in range(0,n):
hν = hν_at(i,n);
value = (hν,sed(hν))
# if (output.value[hν] > max) max = output.value[hν];
# if (output.value[hν] < min) min = output.value[hν];
output.append(value)
# Add a final point at 100 KeV
hν = 1e5;
value = sed(hν);
output.append((hν,value))
return output;
def sed(hν):
magnitude=0.0;
magnitude += powlaw_cutoff(hν,α_HC,E_cutoff_HC,1) # OSSE data fit
if magnitude < CONT_MIN_VAL: return CONT_MIN_VAL
# magnitude = CONT_MIN_VAL;
return magnitude;
def powlaw_cutoff(hν,α,E_cutoff,norm):
low_cutoff = .1
resultant = norm
resultant *= math.exp(-hν/E_cutoff)
resultant *= math.exp(-low_cutoff/hν)
resultant *= math.pow(hν,1+α)
return resultant
# for t in (22.6, 25.8, 27.3, 29.8):+P B
# print(t, ": ", fahrenheit(t))
test_table = histogram_table(500)
for pair in test_table:
print (pair[0],pair[1])