def get_model_func(self):
modellist=[]
ppcross=crss.crossSection(self.ppPath)
counter=0
for p in self.processes:
model=mod.model(self.parentspec[counter],p,self.data,self.source,ppcross)
modellist.append(model.model_val)
counter+=1
return modellist
def fit(self,config=False):
'''
performs the fit of all processes and returns the final
parameter values (list) as well as the model function values
as a list of arrays and the
'''
ppcross=crss.crossSection(self.ppPath)
print 'Setting up fitting routine using:'
print 'evaluating processes %s specs %s with initial parmeters %s'%(self.processes,self.parentspec,self.inPara)
modelfit=fitter.fitter(self.parentspec,self.inPara,self.processes,self.data,self.source,self.confDict,ppcross)
fitFunc=modelfit.fit(config)
#print 'return from fitter in sedfitter: ',fitFunc
'''
Produce finer sampled model functions compared to the fit functions,
these are used for nice plots instead of the data point sampled
graphs that are for test purposes and for the fit
'''
fineGammaY=[]
fineGammaX=[]
counter=0
for p in self.processes:
finalmodel=mod.model(self.parentspec[counter],p,self.data,self.source,ppcross)
finalmodel.set_final_gamma_prec(300)
if p=='pp':
'''
general pp interaction returns secondary emission processes
(Bremsstrahlung and IC) as separated spectra in addition to the pp spectrum and the total spectrum
'''
fineResults=finalmodel.model_val(fitFunc[0][counter])
fineGammaY.append(fineResults[0][0])#total spec
fineGammaY.append(fineResults[0][1])# only pp
fineGammaY.append(fineResults[0][2])# only bremsstrahlung
fineGammaY.append(fineResults[0][3])# only IC
fineGammaX.append(fineResults[1])
fineGammaX.append(fineResults[1])
fineGammaX.append(fineResults[1])
fineGammaX.append(fineResults[1])
counter+=4
else:
fineResults=finalmodel.model_val(fitFunc[0][counter])
fineGammaY.append(fineResults[0])
fineGammaX.append(fineResults[1])
counter+=1
print self.print_fit_results(fitFunc)
return fitFunc+(fineGammaY,fineGammaX)
def plot_sec_spec():
particlePoints=1000
Eg=np.logspace(7.,13.,100)/1.e9
Ee=np.logspace(6.,15.,particlePoints)/1.e9
parameter=[1.,9.,-2.5,10.]
#Ne=spsh.bplcut(Ee,[49.4,-2.43,-2.7,1.69,5.])
Ne=spsh.sbplcuty(Ee,[49.4,1.,-1.5,1.176,-1.4,5.])
#Ne2=spsh.plcut()
ylist=[]
xlist=[]
taglist=[]
elist=[]
ppcrosspath='/Users/jogler/Physik/Fermi/scripts/pp_data/'
ppcross=crs.crossSection(ppcrosspath)
source=sed.source(6000,30.,3.e4)
source.set_radiation_densities(0.25,0.84,3.0e-3,0.9)#W51C densities Abdo et al 2009
source.set_radiation_photons(-8.,4.,0.1)
source.set_am_prop(10.,10.,1.)
fluxScale=Eg/(4.*np.pi*(source.dist*const.PARSEC*const.m2cm)**2.)/const.erg2GeV
print 'Scale: ',fluxScale
pp=mod.model(Ne,'pp',[],source,ppcross)
ppSpec=pp.nucFactor*pp.EdQdE_pp(Ne,Ee,Eg)
#secEPoints=np.logspace(np.log10(Eg[0]),np.log10(Eg[len(Eg)-1]),particlePoints)
eSecSpec=pp.nucFactor*(pp.EdQdE_pp(Ne,Ee,Ee,1)+pp.EdQdE_pp(Ne,Ee,Ee,2))*source.age*const.yr2s
print 'points in secondary spec: ',np.size(eSecSpec)
secBrems=pp.Brems_spec(eSecSpec,Ee,Eg)
secIC=pp.IC_spec_gamma(source.phTot,source.Eph,eSecSpec,Ee,Eg)
ylist.append(ppSpec*fluxScale)
ylist.append(secBrems*fluxScale)
ylist.append(secIC*fluxScale)
xlist.append(Eg)
xlist.append(Eg)
xlist.append(Eg)
elist.append(0)
elist.append(0)
elist.append(0)
taglist.append('pp')
taglist.append('brems sec')
taglist.append('IC sec')
fig=plot(xlist,ylist,[],elist,taglist,r'$\mathrm{E}_{\gamma}\, \mathrm{ [GeV]}$',r'$EF_{\gamma}\, [\mathrm{erg}\, \mathrm{ cm}^{-2} \mathrm{s}^{-1}]$')
plt.show(fig)
def plot_spectrum(typ=['ic','brems','pp']):
'''plots spectra'''
Eg=np.logspace(6.,12.,100)
Ee=np.logspace(6.,15.,1000)
parameter=[1.,9.,-2.5,10.]
#Ne2=spsh.bplcut(Ee,[49.4,-1.5,-2.9,10.176,13.])
Ne2=spsh.sbplcut(Ee,[49.4,9.,-1.5,10.301,2.3,13.])
#print Ne
Ne=spsh.sbplcuty(Ee,[49.4,9.,-1.5,10.301,2.3,13.])#W51C values abdo et al 2009
ENe=Ee*Ne2
spec=sed.spectrum(spsh.sbplcut,[49.4,9.,-1.5,10.301,2.3,13.],1.e6,1.e15,1000.)
#Ne2=spsh.plcut()
ylist=[]
xlist=[]
taglist=[]
elist=[]
source=sed.source()
source.set_radiation_densities(0.25,0.84,3.0e-3,0.9)#W51C densities Abdo et al 2009
source.set_radiation_photons(-8.,4.,0.1)
source.set_am_prop(10.,10.,1.)
ppcrosspath='/Users/jogler/Physik/Fermi/scripts/pp_data/'
ppcross=crs.crossSection(ppcrosspath)
if 'brems' in typ:
brems=mod.model(spec,'brems',[],source,ppcross)
En=brems.spec.get_xvals()*brems.spec.value()
print En-ENe
ylist.append((Eg/1.e9)*brems.Brems_spec(ENe,Ee/1.e9,Eg/1.e9))
#ylist.append(brems.Brems_spec(ENe,Ee/10**9,Eg/10**9))
# ylist.append(brems.Brems_spec_ee(Ne,Ee,Eg))
xlist.append(Eg)
#xlist.append(Eg)
taglist.append('Brems N')
#taglist.append('Brems ee')
elist.append(0)
#elist.append(0)
if 'ic' in typ:
for ph in [source.phTot,source.phCMB,source.phDust,source.phStar]:
ic=mod.model(Ne,'ic',[],source,ppcrosspath)
ylist.append(Eg/1.e9*ic.IC_spec_gamma(ph/source.Eph,source.Eph,ENe,Ee/10**9,Eg/10**9))
xlist.append(Eg)
elist.append(0)
for t in['IC total','IC CMB','IC Dust','IC Star']:
taglist.append(t)
if 'pp' in typ:
pp=mod.model(Ne,'pp',[],source,ppcross)
ylist.append(pp.EdQdE_pp(Ne,Ee/10**9,Eg/10**9))
xlist.append(Eg)
elist.append(0)
taglist.append(r'$\mathrm{pp}_{\gamma} $')
''' plot e+ e- sec spec'''
ylist.append(pp.EdQdE_pp(Ne,Ee/10**9,Eg/10**9,1))
xlist.append(Eg)
elist.append(0)
taglist.append('pp_e-')
ylist.append(pp.EdQdE_pp(Ne,Ee/10**9,Eg/10**9,2))
xlist.append(Eg)
elist.append(0)
taglist.append('pp_e+')
if 'comp' in typ:
if 'brems' in typ:
print 'nH: %.2f nHeff: %.2f Zeff: %.2f'%(source.nH,source.nHeff,source.Zeff)
bremsSp=gs.brems_spectrum(ENe,Ee/10**9,source.nHeff)
ylist.append(Eg/10**9*bremsSp(Eg/10**9))
xlist.append(Eg)
elist.append(0)
taglist.append('brems dima')
if 'ic' in typ:
icSp=gs.IC_spectrum(source.phTot/source.Eph,source.Eph,ENe,Ee/10**9)
ylist.append(Eg/10**9*icSp(Eg/10**9))
xlist.append(Eg)
elist.append(0)
taglist.append('ic dima')
if 'pp' in typ:
ppSp=gs.EdQdE_pp(Ne,Ee/10**9,source.nH,0)
ylist.append(ppSp(Eg/10**9))
xlist.append(Eg)
elist.append(0)
taglist.append('pp dima')
fig0=plot(xlist,ylist,[],elist,taglist,r'$\mathrm{E}_{\gamma}\, \mathrm{ [eV]}$',r'$E^2F_{\gamma}\, [\mathrm{erg}\,\mathrm{ cm}^{-3} \mathrm{s}^{-1}]$')
#plt.show(fig0)
xlist=[]
ylist=[]
elist=[]
taglist=[]
xlist.append(Ee)
xlist.append(Ee)
ylist.append(Ne)
ylist.append(Ne2)
elist.append(0)
elist.append(0)
taglist.append('Ne')
taglist.append('Ne2')
fig1=plot(xlist,ylist,[],elist,taglist,r'$\mathrm{E}_{\gamma}\, \mathrm{ [eV]}$',r'$N_e\, [\mathrm{N}_{e}\mathrm{ cm}^{-3} \mathrm{s}^{-1}]$')
plt.show()
