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#!/usr/bin/env python
import sys
import numpy
import scipy.interpolate
confidence_level=.68
def read_file(param):
delta=float(param[0])
file_mass_center=open("mass_int_center.qdp").readlines();
file_delta_center=open("overdensity_center.qdp").readlines();
center_r=0
center_m=0
center_gm=0
center_gf=0
for i in range(0,len(file_mass_center)):
lm=file_mass_center[i].strip();
ld=file_delta_center[i].strip();
r,m=lm.split()
r,d=ld.split()
r=float(r)
d=float(d)
m=float(m)
if m<1e11:
continue
if d<delta:
center_r=r
center_m=m
for j in open("gas_mass_int_center.qdp"):
rgm,gm=j.strip().split()
rgm=float(rgm)
gm=float(gm)
if rgm>r:
center_gm=gm
center_gf=gm/m
break
break
if len(param)>1 and param[1]=='c':
#print("%s(<r%d)=%E solar mass"%("mass",delta,center_m))
#print("%s%d=%E kpc"%("r",delta,center_r))
#print("%s(<r%d)=%E solar mass"%("gas mass",delta,center_gm))
#print("%s(<r%d)=%E"%("gas fraction",delta,center_gf))
return center_m,center_r,center_gm,center_gf,None,None,None,None
#print(center_gm,center_gf)
file_mass=open('summary_mass_profile.qdp').readlines()
file_delta=open('summary_overdensity.qdp').readlines()
file_gm=open('summary_gas_mass_profile.qdp')
flag=True
rlist=[]
mlist=[]
gmlist=[]
gflist=[]
old_m=0
invalid_count=0
for i in range(0,len(file_mass)):
lm=file_mass[i].strip()
ld=file_delta[i].strip()
if lm[0]=='n':
flag=True
old_m=0
continue
if not flag:
continue
r,m=lm.split()
m=float(m)
if m<1e12:
continue
if m<old_m:
invalid_count+=1
flag=False
continue
r,d=ld.split()
d=float(d)
r=float(r)
if d<delta:
#print("%s %e"%(d,m))
mlist.append(m)
rlist.append(r)
flag1=True
while True:
lgm=file_gm.readline().strip()
if lgm[0]=='n':
break
rgm,gm=lgm.split()
rgm=float(rgm)
gm=float(gm)
if rgm>r and flag1:
gmlist.append(gm)
flag1=False
gflist.append(gm/mlist[-1])
#print(gm,gflist[-1])
flag=False
old_m=m
print("%d abnormal data dropped"%(invalid_count))
return center_m,center_r,center_gm,center_gf,mlist,rlist,gmlist,gflist
#center_m=numpy.mean(mlist)
#center_r=numpy.mean(rlist)
center_m,center_r,center_gm,center_gf,mlist,rlist,gmlist,gflist=read_file(sys.argv[1:])
delta=float(sys.argv[1])
if len(sys.argv)>2 and sys.argv[2]=='c':
print("%s(<r%d)=%E solar mass"%("mass",delta,center_m))
print("%s%d=%E kpc"%("r",delta,center_r))
print("%s(<r%d)=%E solar mass"%("gas mass",delta,center_gm))
print("%s(<r%d)=%E"%("gas fraction",delta,center_gf))
sys.exit(0)
mlist.sort()
rlist.sort()
gflist.sort()
gmlist.sort()
m_idx=-1
r_idx=-1
gm_idx=-1
gf_idx=-1
delta=float(sys.argv[1])
for i in range(len(mlist)-1):
if (center_m-mlist[i])*(center_m-mlist[i+1])<=0:
m_idx=i
break
for i in range(len(rlist)-1):
if (center_r-rlist[i])*(center_r-rlist[i+1])<=0:
r_idx=i
break
for i in range(len(gmlist)-1):
if (center_gm-gmlist[i])*(center_gm-gmlist[i+1])<=0:
gm_idx=i
break
for i in range(len(gflist)-1):
if (center_gf-gflist[i])*(center_gf-gflist[i+1])<=0:
gf_idx=i
break
if m_idx==-1 or r_idx==-1 or gf_idx==-1 or gm_idx==-1:
print("Error, the center value is not enclosed by the Monte-Carlo realizations, please check the result!")
print("m:%E %E %E"%(center_m,mlist[0],mlist[-1]))
print("gm:%E %E %E"%(center_gm,gmlist[0],gmlist[-1]))
print("gf:%E %E %E"%(center_gf,gflist[0],gflist[-1]))
print("r:%E %E %E"%(center_r,rlist[0],rlist[-1]))
sys.exit(1)
mlidx=int(m_idx*(1-confidence_level))
muidx=m_idx-1+int((len(mlist)-m_idx)*confidence_level)
rlidx=int(r_idx*(1-confidence_level))
ruidx=r_idx-1+int((len(rlist)-r_idx)*confidence_level)
gmlidx=int(gm_idx*(1-confidence_level))
gmuidx=gm_idx-1+int((len(gmlist)-gm_idx)*confidence_level)
gflidx=int(gf_idx*(1-confidence_level))
gfuidx=gf_idx-1+int((len(gflist)-gf_idx)*confidence_level)
merr1=mlist[mlidx]-center_m
merr2=mlist[muidx]-center_m
rerr1=rlist[rlidx]-center_r
rerr2=rlist[ruidx]-center_r
gmerr1=gmlist[gmlidx]-center_gm
gmerr2=gmlist[gmuidx]-center_gm
gferr1=gflist[gflidx]-center_gf
gferr2=gflist[gfuidx]-center_gf
#print("%d %d %d"%(mlidx,m_idx,muidx))
#print("%d %d %d"%(rlidx,r_idx,ruidx))
print("m%d=\t%e\t %e/+%e solar mass (1 sigma)"%(delta,center_m,merr1,merr2))
print("gas_m%d=\t%e\t %e/+%e solar mass (1 sigma)"%(delta,center_gm,gmerr1,gmerr2))
print("gas_fraction%d=\t%e\t %e/+%e (1 sigma)"%(delta,center_gf,gferr1,gferr2))
print("r%d=\t%d\t %d/+%d kpc (1 sigma)"%(delta,center_r,rerr1,rerr2))
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