zmaxlist = map(float, zrArr['zmax'])
minz = np.min(zminlist)
maxz = np.max(zmaxlist)
#maxz = np.max(zrArr['zmax'])
print minz, maxz
minsfr = 10.0
print 'loading lightcone data'
GalArr, lLyc, ngg, DistNz, zspace = readmock(zmin=minz,
zmax=maxz,
sfrmin=minsfr,
zspace=1)
print 'now loading photo-ionisation grid'
lineinfo, linesarr = read_photoion()
qpar = qZrelation(GalArr['Zcold']) # assuming default pars.
#loii_1 = np.zeros(ngg,dtype=np.float32)
#loii_2 = np.zeros(ngg,dtype=np.float32)
print 'Computing emission line(s)'
def get_all_oii(i):
#for i in range(ngg):
loii_1 = integ_line(lineinfo, linesarr, qpar[i], GalArr['Zcold'][i],
lLyc[i], 'OII_3727')
loii_2 = integ_line(lineinfo, linesarr, qpar[i], GalArr['Zcold'][i],
lLyc[i], 'OII_3729')
def main(nproc, outfile):
"""
Creates files containing all emission line luminosities and
magnitudes for lightcone galaxies.
Calculation is split in a given number of processes, where
each computes the emission lines of a chunk of data independently
and outputs the results to a file.
Arguments:
nproc = number of processes
outfile = Output file name. (final name will be followed by a number)
"""
# nproc = argv[0]
# outfile = argv[1]
# if (len(argv) < 2):
# print 'you need to provide 2 arguments: nproc outfile.'
# print 'Exiting..'
# return 0
nproc = int(nproc)
IncludeMags = True
print 'nproc:', nproc, ' outfile:', outfile
sys.stdout.flush()
#L_line = 1215.67 # Angstroms
L_line = 3727.0 # Angstroms
#Lyaz,izr,GalArr,Vol = get_lya(zrange)
FiltArr, wrange = rf.read_filters()
jpaslims = jp.get_jpaslims()
app_type = 1 # 0 means per 3 arcsec diameter, 1 means per square arcsec
cosmo = FlatLambdaCDM(H0=73, Om0=0.25)
zrArr = comparat_zranges()
zminlist = map(float, zrArr['zmin'])
zmaxlist = map(float, zrArr['zmax'])
minz = np.min(zminlist)
maxz = np.max(zmaxlist)
#maxz = np.max(zrArr['zmax'])
print minz, maxz
minsfr = 0.1
nFil = len(FiltArr['w'])
CentralW = np.zeros(nFil)
int_ab = np.zeros(nFil)
p10p90W = np.zeros([nFil, 2])
for i in range(nFil):
CentralW[i] = wp.quantile(FiltArr['w'][i], FiltArr['t'][i], 0.5)
nz = np.where(FiltArr['w'][i] != 0)
int_ab[i] = (integral.simps(FiltArr['t'][i][nz] / FiltArr['w'][i][nz],
FiltArr['w'][i][nz]))
p10p90W[i, 0] = wp.quantile(FiltArr['w'][i][nz], FiltArr['t'][i][nz],
0.1)
p10p90W[i, 1] = wp.quantile(FiltArr['w'][i][nz], FiltArr['t'][i][nz],
0.9)
print 'int_ab[i]', int_ab[i]
print 'loading lightcone data'
props = ['redshift', 'pos', 'Mz', 'Mcold', 'sfr', 'vel', 'stellarmass']
print 'now loading photo-ionisation grid'
lineinfo, linesarr = read_photoion()
nline = lineinfo['nlines']
usezspace = 1
# magtype stores both the value of the magnitude (float) and the
# filter id (int) where that magnitude was computed.
magtype = np.dtype('f4, i4')
def read_lightcone_chunk(ip, nproc):
GalArr, lLyc, ngg, DistNz, zdist = readmock_chunk(ip,
nproc,
props_array=props,
zspace=usezspace,
sfrmin=500)
zcold = GalArr['Mcold'] / GalArr['Mz']
qpar = qZrelation(zcold) # assuming default pars.
# This stores all line luminosities for all galaxies
# LinesLumArr[i,j] = Luminosity of line j for galaxy i.
LinesLumArr = np.zeros((ngg, nline))
redshiftArr = np.zeros(ngg)
SfrArr = np.zeros(ngg)
MStellarArr = np.zeros(ngg)
ZArr = np.zeros(ngg)
print 'ip ' + str(
ip) + ', computing lines for ngals=', ngg, ' galaxies...'
sys.stdout.flush()
for ig in range(ngg):
LinesLumArr[ig, :] = integ_line(lineinfo,
linesarr,
qpar[ig],
zcold[ig],
lLyc[ig],
all_lines=True)
redshiftArr[ig] = GalArr['redshift'][ig]
SfrArr[ig] = GalArr['sfr'][ig]
MStellarArr[ig] = GalArr['stellarmass'][ig]
ZArr[ig] = zcold[ig]
# LinesLumArr[ig,il] = iline
print 'redshiftArr', redshiftArr[0:10]
print 'Lines[0,:]', LinesLumArr[0, :]
print 'Lines[10,:]', LinesLumArr[10, :]
print 'Lines[100,:]', LinesLumArr[100, :]
print 'zarr[100,:]', ZArr[0:100]
print 'Proc ip:' + str(ip) + ' done with that.'
# This stores the AB observed-frame apparent magnitude for all luminosities of all galaxies, indicating also to which filter
# the stored magnitudes corresponds to.
# MagsLumArr[i,j] = (AB magnitude, filter id) of line j of galaxy i.
MagsLumArr = np.zeros((ngg, nline), dtype=magtype)
realdist = np.sqrt(GalArr['pos'][:, 0]**2 + GalArr['pos'][:, 1]**2 +
GalArr['pos'][:, 2]**2)
log_dist = np.log10(realdist) + np.log10(mpc2cm_24) + 24.0 + np.log10(
1 + GalArr['redshift'])
if IncludeMags is True:
for il in range(nline):
L_line = lineinfo['lambda0'][il]
wgal = L_line * (1 + GalArr['redshift'])
log_Fline = LinesLumArr[:, il] - (np.log10(4 * np.pi) + 2 *
(log_dist))
FLine = 10**log_Fline
for i in range(ngg):
idFilter, Val = find_nearest_vector(CentralW, wgal[i])
if idFilter == 0:
if wgal[i] < p10p90W[0, 0]:
MagsLumArr[i, il] = (-99, -99)
continue
elif idFilter == nFil - 1:
if wgal[i] > p10p90W[nFil - 1, 1]:
MagsLumArr[i, il] = (99, 99)
continue
else:
nz = np.where(FiltArr['w'][idFilter] != 0)
lamb = FiltArr['w'][idFilter][nz]
tlamb = FiltArr['t'][idFilter][nz]
tlam0 = np.interp(wgal[i], lamb, tlamb)
# mag_app[i] = -2.5*(log_Fline[i]+ np.log10((wgal[i]*tlam0)/int_ab[idFilter]) - 18-np.log10(3.0)) - 48.60
mag_app = -2.5 * (log_Fline[i] + np.log10(
(wgal[i] * tlam0) / int_ab[idFilter]) - 18 -
np.log10(3.0)) - 48.60
MagsLumArr[i, il] = (mag_app, idFilter)
filename = outfile + '.' + str(ip)
nf = open(filename, "wb")
print 'writing file ' + filename
nf.write(struct.pack('l', ngg))
nf.write(struct.pack('i', nline))
LinesLumArr.tofile(nf)
if IncludeMags is True:
MagsLumArr.tofile(nf)
redshiftArr.tofile(nf)
SfrArr.tofile(nf)
MStellarArr.tofile(nf)
ZArr.tofile(nf)
nf.close()
print 'file ' + filename + ' written succesfully.'
return 1
if nproc == 1:
processes = read_lightcone_chunk(0, 1)
else:
print 'start processes'
processes = [
mp.Process(target=read_lightcone_chunk, args=(ip, nproc))
for ip in range(nproc)
]
for p in processes:
p.start()
for p in processes:
p.join()
return 1
minz = np.min(zminlist) maxz = np.max(zmaxlist) #maxz = np.max(zrArr['zmax']) print minz,maxz minsfr = 5.0 print 'loading lightcone data' sys.stdout.flush() props = ['redshift','pos','Zcold','sfr','vel'] GalArr,lLyc,ngg,DistNz,zspace = readmock(props_array = props, zmin=minz,zmax=maxz, sfrmin=minsfr,zspace=1) ngals = ngg print 'now loading photo-ionisation grid' lineinfo,linesarr = read_photoion() qpar = qZrelation(GalArr['Zcold']) # assuming default pars. #loii_1 = np.zeros(ngg,dtype=np.float32) #loii_2 = np.zeros(ngg,dtype=np.float32) print 'Computing emission line(s)' sys.stdout.flush() def get_all_oii(i): #for i in range(ngg): loii_1 = integ_line(lineinfo,linesarr,qpar[i],GalArr['Zcold'][i],lLyc[i],'OII_3727') loii_2 = integ_line(lineinfo,linesarr,qpar[i],GalArr['Zcold'][i],lLyc[i],'OII_3729') if i == ngg/10: print '.10%' if i == ngg/5:
def main(nproc,outfile):
"""
Creates files containing all emission line luminosities and
magnitudes for lightcone galaxies.
Calculation is split in a given number of processes, where
each computes the emission lines of a chunk of data independently
and outputs the results to a file.
Arguments:
nproc = number of processes
outfile = Output file name. (final name will be followed by a number)
"""
# nproc = argv[0]
# outfile = argv[1]
# if (len(argv) < 2):
# print 'you need to provide 2 arguments: nproc outfile.'
# print 'Exiting..'
# return 0
nproc = int(nproc)
IncludeMags = True
print 'nproc:',nproc,' outfile:',outfile
sys.stdout.flush()
#L_line = 1215.67 # Angstroms
L_line = 3727.0 # Angstroms
#Lyaz,izr,GalArr,Vol = get_lya(zrange)
FiltArr,wrange = rf.read_filters()
jpaslims = jp.get_jpaslims()
app_type = 1 # 0 means per 3 arcsec diameter, 1 means per square arcsec
cosmo = FlatLambdaCDM(H0=73, Om0=0.25)
zrArr = comparat_zranges()
zminlist = map(float,zrArr['zmin'])
zmaxlist = map(float,zrArr['zmax'])
minz = np.min(zminlist)
maxz = np.max(zmaxlist)
#maxz = np.max(zrArr['zmax'])
print minz,maxz
minsfr = 0.1
nFil = len(FiltArr['w'])
CentralW = np.zeros(nFil)
int_ab = np.zeros(nFil)
p10p90W = np.zeros([nFil,2])
for i in range(nFil):
CentralW[i] = wp.quantile(FiltArr['w'][i],FiltArr['t'][i],0.5)
nz = np.where(FiltArr['w'][i] != 0)
int_ab[i] = (integral.simps(FiltArr['t'][i][nz]/FiltArr['w'][i][nz],FiltArr['w'][i][nz]))
p10p90W[i,0] = wp.quantile(FiltArr['w'][i][nz],FiltArr['t'][i][nz],0.1)
p10p90W[i,1] = wp.quantile(FiltArr['w'][i][nz],FiltArr['t'][i][nz],0.9)
print 'int_ab[i]',int_ab[i]
print 'loading lightcone data'
props = ['redshift','pos','Mz','Mcold','sfr','vel','stellarmass']
print 'now loading photo-ionisation grid'
lineinfo,linesarr = read_photoion()
nline = lineinfo['nlines']
usezspace = 1
# magtype stores both the value of the magnitude (float) and the
# filter id (int) where that magnitude was computed.
magtype = np.dtype('f4, i4')
def read_lightcone_chunk(ip, nproc):
GalArr,lLyc,ngg,DistNz,zdist = readmock_chunk(ip,nproc,props_array = props,
zspace=usezspace,sfrmin=500)
zcold = GalArr['Mcold']/GalArr['Mz']
qpar = qZrelation(zcold) # assuming default pars.
# This stores all line luminosities for all galaxies
# LinesLumArr[i,j] = Luminosity of line j for galaxy i.
LinesLumArr = np.zeros((ngg,nline))
redshiftArr = np.zeros(ngg)
SfrArr = np.zeros(ngg)
MStellarArr = np.zeros(ngg)
ZArr = np.zeros(ngg)
print 'ip '+str(ip)+', computing lines for ngals=',ngg,' galaxies...'
sys.stdout.flush()
for ig in range(ngg):
LinesLumArr[ig,:] = integ_line(lineinfo,linesarr,qpar[ig],zcold[ig],lLyc[ig],all_lines=True)
redshiftArr[ig] = GalArr['redshift'][ig]
SfrArr[ig] = GalArr['sfr'][ig]
MStellarArr[ig] = GalArr['stellarmass'][ig]
ZArr[ig] = zcold[ig]
# LinesLumArr[ig,il] = iline
print 'redshiftArr' , redshiftArr[0:10]
print 'Lines[0,:]' , LinesLumArr[0,:]
print 'Lines[10,:]' , LinesLumArr[10,:]
print 'Lines[100,:]' , LinesLumArr[100,:]
print 'zarr[100,:]' , ZArr[0:100]
print 'Proc ip:'+str(ip)+' done with that.'
# This stores the AB observed-frame apparent magnitude for all luminosities of all galaxies, indicating also to which filter
# the stored magnitudes corresponds to.
# MagsLumArr[i,j] = (AB magnitude, filter id) of line j of galaxy i.
MagsLumArr = np.zeros((ngg,nline),dtype=magtype)
realdist = np.sqrt(GalArr['pos'][:,0]**2 + GalArr['pos'][:,1]**2+GalArr['pos'][:,2]**2)
log_dist = np.log10(realdist) + np.log10(mpc2cm_24)+24.0 + np.log10(1+GalArr['redshift'])
if IncludeMags is True:
for il in range(nline):
L_line = lineinfo['lambda0'][il]
wgal = L_line*(1 + GalArr['redshift'])
log_Fline = LinesLumArr[:,il] - (np.log10(4*np.pi)+2*(log_dist))
FLine = 10**log_Fline
for i in range(ngg):
idFilter,Val = find_nearest_vector(CentralW,wgal[i])
if idFilter == 0:
if wgal[i] < p10p90W[0,0]:
MagsLumArr[i,il] = (-99,-99)
continue
elif idFilter == nFil-1:
if wgal[i] > p10p90W[nFil-1,1]:
MagsLumArr[i,il] = (99,99)
continue
else:
nz = np.where(FiltArr['w'][idFilter] != 0)
lamb = FiltArr['w'][idFilter][nz]
tlamb = FiltArr['t'][idFilter][nz]
tlam0 = np.interp(wgal[i],lamb,tlamb)
# mag_app[i] = -2.5*(log_Fline[i]+ np.log10((wgal[i]*tlam0)/int_ab[idFilter]) - 18-np.log10(3.0)) - 48.60
mag_app = -2.5*(log_Fline[i]+ np.log10((wgal[i]*tlam0)/int_ab[idFilter]) - 18-np.log10(3.0)) - 48.60
MagsLumArr[i,il] = (mag_app, idFilter)
filename = outfile + '.' + str(ip)
nf = open(filename,"wb")
print 'writing file '+filename
nf.write(struct.pack('l',ngg))
nf.write(struct.pack('i',nline))
LinesLumArr.tofile(nf)
if IncludeMags is True:
MagsLumArr.tofile(nf)
redshiftArr.tofile(nf)
SfrArr.tofile(nf)
MStellarArr.tofile(nf)
ZArr.tofile(nf)
nf.close()
print 'file '+filename+' written succesfully.'
return 1
if nproc == 1:
processes = read_lightcone_chunk(0,1)
else:
print 'start processes'
processes = [mp.Process(target=read_lightcone_chunk, args=(ip,nproc)) for ip in range(nproc)]
for p in processes:
p.start()
for p in processes:
p.join()
return 1