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##############################################################################
# CREATION OF LIBRARIES FROM SEDs List #
# $LEPHAREDIR/source/sedtolib -t (S/Q/G) -c $LEPHAREDIR/config/zphot.para #
# help : $LEPHAREDIR/source/sedtolib -h (or -help) #
##############################################################################
#
#------ STELLAR LIBRARY (ASCII SEDs)
STAR_SED $LEPHAREDIR/sed/STAR/STAR_MOD.list # STAR list (full path)
STAR_FSCALE 3.432E-09 # Arbitrary Flux Scale
STAR_LIB LIB_STAR # Bin. STAR LIBRARY ->
# $LEPHAREWORK/lib_bin
#
#------ QSO LIBRARY (ASCII SEDs)
QSO_SED $LEPHAREDIR/sed/QSO/QSO_MOD.list # QSO list (full path)
QSO_FSCALE 1 # Arbitrary Flux Scale
QSO_LIB LIB_QSO # Bin. QSO LIBRARY ->
# $LEPHAREWORK/lib_bin
#
#------ GALAXY LIBRARY (ASCII or BINARY SEDs)
GAL_SED $LEPHAREDIR/sed/GAL/CWW_KINNEY/CWW_MOD.list # GAL list (full path)
GAL_FSCALE 1. # Arbitrary Flux Scale
GAL_LIB LIB_CWW # Bin. GAL LIBRARY ->
# $LEPHAREWORK/lib_bin
#SEL_AGE $LEPHAREDIR/sed/GAL/HYPERZ/AGE_GISSEL_ALL.dat # Age list(full path)
# (def=NONE)
AGE_RANGE 0.,13.e9 # Age Min-Max in yr
#
#############################################################################
# FILTERS #
# $LEPHAREDIR/source/filter -c $LEPHAREDIR/config/zphot.para #
# help: $LEPHAREDIR/source/filter -h (or -help) #
#############################################################################
# Filter number and context
# f275 f435 f606 f775 f814 f850lp f105 f125 f140 f160
# 1 2 3 4 5 6 7 8 9 10
# 1 2 4 8 16 32 64 128 256 512= 511
#
FILTER_LIST hst_candles/f275w.dat,hst_candles/f435w.dat,hst_candles/f606w.dat,hst_candles/f775w.dat,hst_candles/f814w.dat,hst_candles/f850lp.dat,hst_candles/f105w.dat,hst_candles/f125w.dat,hst_candles/f140w.dat,hst_candles/f160w.dat
# (in $LEPHAREDIR/filt/*)
TRANS_TYPE 0 # TRANSMISSION TYPE
# 0[-def]: Energy, 1: Nb of photons
FILTER_CALIB 0 # 0[-def]: fnu=ctt
# 1 : nu.fnu=ctt
# 2 : fnu=nu
# 3 : fnu=Black Body @ T=10000K
# 4 : for MIPS (leff with nu fnu=ctt and flux with BB @ 10000K
FILTER_FILE cosmos.filt # output name of filter's file ->
# $LEPHAREWORK/filt/
#
############################################################################
# THEORETICAL MAGNITUDES #
# $LEPHAREDIR/source/mag_star -c $LEPHAREDIR/config/zphot.para (star only)#
# help: $LEPHAREDIR/source/mag_star -h (or -help) #
# $LEPHAREDIR/source/mag_gal -t (Q or G) -c $LEPHAREDIR/config/zphot.para #
# (for gal. & QSO) #
# help: $LEPHAREDIR/source/mag_gal -h (or -help) #
############################################################################
#
#------- From STELLAR LIBRARY
STAR_LIB_IN LIB_STAR # Input STELLAR LIBRARY in $LEPHAREWORK/lib_bin/
STAR_LIB_OUT STAR_HDF # Output STELLAR MAGN -> $LEPHAREWORK/lib_mag/
#
#------- From QSO LIBRARY
QSO_LIB_IN LIB_QSO # Input QSO LIBRARY in $LEPHAREWORK/lib_bin/
QSO_LIB_OUT QSO_HDF # Output QSO MAGN -> $LEPHAREWORK/lib_mag/
#
#------- From GALAXY LIBRARY
GAL_LIB_IN LIB_CWW # Input GAL LIBRARY in $LEPHAREWORK/lib_bin/
GAL_LIB_OUT CWW_HDF # Output GAL LIBRARY -> $LEPHAREWORK/lib_mag/
#
#------- MAG + Z_STEP + EXTINCTION + COSMOLOGY
MAGTYPE AB # Magnitude type (AB or VEGA)
Z_STEP 0.04,6.,0.1 # dz, zmax, dzsup(if zmax>6)
COSMOLOGY 70,0.3,0.7 # H0,om0,lbd0 (if lb0>0->om0+lbd0=1)
MOD_EXTINC 13,23,23,31,23,31,23,31 # model range for extinction
EXTINC_LAW SMC_prevot.dat,SB_calzetti.dat,SB_calzetti_bump1.dat,SB_calzetti_bump2.dat # ext. law (in $LEPHAREDIR/ext/*)
EB_V 0.000,0.100,0.200,0.300,0.400,0.500 # E(B-V) (<50 values)
EM_LINES YES
# Z_FORM 8,7,6,5,4,3 # Zformation for each SED in GAL_LIB_IN
#
#------- ASCII OUTPUT FILES OPTION
LIB_ASCII NO # Writes output in ASCII
# in working directory
#
############################################################################
# PHOTOMETRIC REDSHIFTS #
# $LEPHAREDIR/source/zphot -c $LEPHAREDIR/config/zphot.para #
# help: $LEPHAREDIR/source/zphot -h (or -help) #
############################################################################
#
#
#
#------- Input Catalog Informations
CAT_IN $LEPHAREWORK/tst.in # Input catalog (full path)
INP_TYPE M # Input type (F:Flux or M:MAG)
CAT_MAG AB # Input Magnitude (AB or VEGA)
CAT_FMT MEME # MEME: (Mag,Err)i
# MMEE: (Mag)i,(Err)i
CAT_LINES -99,-99 # MIN and MAX RANGE of ROWS used in input cat [def:-99,-99]
CAT_TYPE LONG # Input Format (LONG,SHORT-def)
CAT_OUT $LEPHAREWORK/test/zphot_1.out # Output catalog (full path)
PARA_OUT $LEPHAREWORK/config/zphot_output.para # Ouput parameter (full path)
#
BD_SCALE 0 # Bands used for scaling
# (Sum 2^n; n=0->nbd-1, 0[-def]:all bands)
GLB_CONTEXT -1 # Overwrite Context (Sum 2^n; n=0->nbd-1,
# 0 : all bands used,
# -1[-def]: used context per object
# FORB_CONTEXT -1 # context for forbitten bands
ERR_SCALE 0.03,0.02,0.02,0.02,0.04 # errors per band added in quadrature
ERR_FACTOR 1.0 # error scaling factor 1.0 [-def]
#
#------- Theoretical libraries
ZPHOTLIB CWW_HDF,STAR_HDF,QSO_HDF # Library used for Chi2 (max:3)
ADD_EMLINES YES
#
######## PHOTOMETRIC REDSHIFTS OPTIONS ###########
# FIR LIBRARY
FIR_LIB NONE
FIR_LMIN 7.0 # Lambda Min (micron) for FIR analysis
FIR_CONT -1
FIR_SCALE -1
FIR_FREESCALE YES # ALLOW FOR FREE SCALING
FIR_SUBSTELLAR NO
# PHYSICAL LIBRARY with Stochastic models from BC07
PHYS_LIB NONE
PHYS_CONT -1
PHYS_SCALE -1
PHYS_NMAX 100000
#
#------- Priors
# MASS_SCALE 6.,16. # Lg(Scaling) min,max [0,0-def]
MAG_ABS -10.,-26. # Mabs_min , Mabs_max [0,0-def]
MAG_REF 4 # Reference number for band used by Mag_abs
# ZFORM_MIN 5,5,5,5,5,5,3,1 # Min. Zformation per SED -> Age constraint
Z_RANGE 0.,99.99 # Z min-max used for the Galaxy library
EBV_RANGE 0,9 # E(B-V) MIN-MAX RANGE of E(B-V) used
# NZ_PRIOR 4,2,4 # I Band for prior on N(z)
#
#------- Fixed Z (need format LONG for input Cat)
ZFIX YES # fixed z and search best model [YES,NO-def]
#
#------- Parabolic interpolation for Zbest
Z_INTERP YES # redshift interpolation [YES,NO-def]
#
#------- Analysis of normalized ML(exp-(0.5*Chi^2)) curve
#------- Secondary peak analysis
DZ_WIN 0.5 # Window search for 2nd peaks [0->5;0.25-def]
MIN_THRES 0.1 # Lower threshold for 2nd peaks[0->1; 0.1-def]
#
#------- Probability (in %) per redshift intervals
# PROB_INTZ 0,0.5,0.5,1.,1.,1.5 # even number
#
######### ABSOLUTE MAGNITUDES COMPUTATION ###########
#
MABS_METHOD 1 # 0[-def] : obs->Ref
# 1 : best obs->Ref
# 2 : fixed obs->Ref
# 3 : mag from best SED
# 4 : Zbin
MABS_CONTEXT -1 # CONTEXT for Band used for MABS
MABS_REF 4 # 0[-def]: filter obs chosen for Mabs :
# ONLY USED IF MABS_METHOD=2
MABS_FILT 1,2,3,4 # Chosen filters per redshift bin (MABS_ZBIN)
# ONLY USED IF MABS_METHOD=4
MABS_ZBIN 0,0.5,1,1.5,2,3,3.5,4 # Redshift bins (even number)
# ONLY USED IF MABS_METHOD=4
######### OUTPUT SPECTRA ###########
#
SPEC_OUT YES # spectrum for each object? [YES,NO-def]
CHI2_OUT NO # output file with all values : z,mod,chi2,E(B-V),...
# BE CAREFUL can take a lot of space !!
######### OUTPUT PDZ ANALYSIS
PDZ_OUT NONE # pdz output file name [def-NONE]
# add automatically PDZ_OUT[.pdz/.mabsx/.mod/.zph]
PDZ_MABS_FILT 2,10,14 # MABS for REF FILTERS to be extracted
#
######### FAST MODE : color-space reduction #####
#
FAST_MODE NO # Fast computation [NO-def]
COL_NUM 3 # Number of colors used [3-def]
COL_SIGMA 3 # Enlarge of the obs. color-errors[3-def]
COL_SEL AND # Combination between used colors [AND/OR-def]
#
######### MAGNITUDE SHIFTS applied to libraries ######
#
# APPLY_SYSSHIFT 0. # Apply systematic shifts in each band
# used only if number of shifts matches
# with number of filters in the library
#
######### ADAPTIVE METHOD using Z spectro sample ###
#
AUTO_ADAPT NO # Adapting method with spectro [NO-def]
ADAPT_BAND 4,2,4 # Reference band, band1, band2 for color
ADAPT_LIM 18,22.0 # Mag limits for spectro in Ref band [18,21.5-def]
ADAPT_POLY 1 # Number of coef in polynom (max=4) [1-def]
ADAPT_METH 1 # Fit as a function of
# 1 : Color Model [1-def]
# 2 : Redshift
# 3 : Models
ADAPT_CONTEXT -1 # Context for bands used for training
# -1[-def] used context per object
ADAPT_ZBIN 0.01,6 # Redshift's interval used for training
# [0.001,6-Def]
ADAPT_MODBIN 1,1000 # Model's interval used for training
# [1,1000-Def]
ERROR_ADAPT NO # [YES,NO-def]
# Add error in quadrature according to
# the difference between observed
# and predicted apparent magnitudes
#
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#######################################
# PHOTOMETRIC REDSHIFT with OPTIONS #
# Input catalog #
# CAT_IN : /Users/zhangxin/Work/SED_PRJ/superSim//outData/lp/spec/9386/iso.cat-CAT_OUT
# CAT_LINES : -99 -99
# INP_TYPE : M
# CAT_MAG : AB
# CAT_FMT[0:MEME 1:MMEE]: 0
# Input library #
# FILTER_FILE : candles.filt
# AB 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00
# 1.572 -0.080 0.091 0.403 0.436 0.537 0.651 0.908 1.084 1.270
# ZPHOTLIB : CWW_HDF
# using : LIB_CWW
# ADD_EMLINES : YES
# Z_STEP : 0.04 3.00 0.10
# CHI2_RM_BD : 10000.00 10000.00
# Z_RANGE : 0.000 99.990
# EBV_RANGE : 0.200 0.900
# Z_INTERP : YES
# COSMOLOGY : 70.00 0.30 0.70
# EXTINC_LAW : SMC_prevot.dat SB_calzetti.dat SB_calzetti_bump1.dat SB_calzetti_bump2.dat
# EB_V : 0.000 0.100 0.200 0.300 0.400 0.500
# MOD_EXTINC : 13 23 23 31 23 31 23 31
# FAST_MODE : NO
# ERR_SCALE : -1.000 -1.000 -1.000 -1.000 -1.000
# ERR_FACTOR : 1.000
# Options #
# BD_SCALE : 0
# GLB_CONTEXT : 0
# DZ_WIN : 0.500
# MIN_THRES : 0.100
# MASS_SCALE : 0.00 0.00
# MAG_ABS : -10.00 -26.00
# MAG_REF : 4
# PROB_INTZ : 0.000
# MABS_METHOD : 1
# MABS_CONTEXT: -1
# MABS_REF : 4
# AUTO_ADAPT : NO
# NZ_PRIOR : 0 0 0
# ZFIX : YES
# SPEC_OUT : YES
# CHI2_OUT : NO
# PDZ_OUT : NONE
# CAT_OUT : /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//config/zphot_1.out
# PARA_OUT : /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//config/zphot_output.para
# CREATION_DATE: Wed Mar 16 13:31:06 2022
# Output format #
# IDENT 1 , Z_BEST 2 , Z_ML 3 , CHI_BEST 4 , MOD_BEST 5 ,
# EXTLAW_BEST 6 , EBV_BEST 7 , PDZ_BEST 8 , CONTEXT 9 , ZSPEC 10 ,
# STRING_INPUT 10 ,
#######################################
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IDENT
Z_BEST
#Z_BEST68_LOW
#Z_BEST68_HIGH
Z_ML
#Z_ML68_LOW
#Z_ML68_HIGH
#Z_BEST90_LOW
#Z_BEST90_HIGH
#Z_BEST99_LOW
#Z_BEST99_HIGH
CHI_BEST
MOD_BEST
EXTLAW_BEST
EBV_BEST
#ZF_BEST
#MAG_ABS_BEST
PDZ_BEST
#SCALE_BEST
#DIST_MOD_BEST
#NBAND_USED
#NBAND_ULIM
#
####### Z-2nd GALAXY ###########
#Z_SEC
#CHI_SEC
#MOD_SEC
#AGE_SEC
#EBV_SEC
#ZF_SEC
#MAG_ABS_SEC
#PDZ_SEC
#SCALE_SEC
#
######## Z-Best QSO #############
#Z_QSO
#CHI_QSO
#MOD_QSO
#MAG_ABS_QSO
#DIST_MOD_QSO
######## Best STAR #############
#MOD_STAR
#CHI_STAR
#
######## OBSERVED MAGNITUDES ####
#MAG_OBS()
#ERR_MAG_OBS()
######## MODEL MAGNITUDES FOR GALAXY ####
#MAG_MOD()
#
######## K-COR , ABSOLUTE MAG, FILTER CHOICE FOR GALAXY ##########
#K_COR()
#MAG_ABS()
#MABS_FILT()
#
######## K-COR , ABSOLUTE MAG. FOR QSO ##########
#K_COR_QSO()
#MAG_ABS_QSO()
#
####### PROBABILITY PER Z BINS ##
#PDZ()
#
####### INPUT INFO ##############
CONTEXT
ZSPEC
STRING_INPUT
####### Far-IR PARAMETERS derived from FIR_LIB library ###########
#LUM_TIR_BEST
#LIB_FIR
#MOD_FIR
#CHI2_FIR
#FSCALE_FIR
#NBAND_FIR
#LUM_TIR_MED
#LUM_TIR_INF
#LUM_TIR_SUP
#MAG_MOD_FIR()
#MAG_ABS_FIR()
#K_COR_FIR()
######### PHYSICAL PARAMETERS derived from ZPHOTLIB library IF DEFINED ######
#AGE_BEST
#AGE_INF
#AGE_MED
#AGE_SUP
##
#LDUST_BEST
#LDUST_INF
#LDUST_MED
#LDUST_SUP
##
#MASS_BEST
#MASS_INF
#MASS_MED
#MASS_SUP
#
#SFR_BEST
#SFR_INF
#SFR_MED
#SFR_SUP
#
#SSFR_BEST
#SSFR_INF
#SSFR_MED
#SSFR_SUP
#
#LUM_NUV_BEST
#LUM_R_BEST
#LUM_K_BEST
######### PHYSICAL PARAMETERS derived from PHYS_LIB library
# best Chi^2 or median+/-68% of the ML distribution
# 1: Lg(Age[yr]) [1]
# 2: Lg(Lnuv[Lo]) [23] 3: Lg(Lr[Lo]) [24]
# 4: Lg(Lk[Lo]) [25]
# 5: Lg(Ldust[Lo]) [5] 6: Lg(Mass[Mo]) [6]
# 7: Lg(SFR_1e8[Mo/yr]) [8] 8: Lg(SFR_1e9[Mo/yr]) [9]
# 9: Gamma[Gyr] [10] 10: Metallicity [11]
# 11: Tauv [12] 12: mu [13]
# 13: Lg(Age_weightmass[yr])[14] 14: Lg(Age_weightLr[yr]) [15]
# 15: Lg(Age_Tlastburst[yr])[16]
# 16: Frac_burst<1.e8[yr] [17] 17: Frac_burst<1e9[yr] [18]
# 18: Nb burst [21]
# 19: Lg(SSFR_1e8 [yr-1]) [42] 20: Lg(SSFR_1e9 [yr-1]) [43]
# 21: A(1500) [mag] [26] 22: A(2300) [mag] [27]
# 23: A(4500) [mag] [29] 24: A(6000) [mag] [30]
# 25: A(8500) [mag] [31] 26: A(22000)[mag] [32]
# 27: A(3500) [mag] [28]
# 28: D4000 [34] 29: Lg(Ldust_LC00) [39]
# 30: F_mu[Ld(ISM)/Ld_LC00] [40] 31: eta[Ld(>4000)/Ld)] [41]
# 32: Rec_Mass[(Mt-M*)/Mt] [7]
#####################################################
#PHYS_CHI2_BEST
#PHYS_MOD_BEST
#PHYS_MAG_MOD()
#PHYS_MAG_ABS()
#PHYS_K_COR()
#PHYS_PARA1_BEST
#PHYS_PARA2_BEST
#PHYS_PARA3_BEST
#PHYS_PARA4_BEST
#PHYS_PARA5_BEST
#PHYS_PARA6_BEST
#PHYS_PARA7_BEST
#PHYS_PARA8_BEST
#PHYS_PARA9_BEST
#PHYS_PARA10_BEST
#PHYS_PARA11_BEST
#PHYS_PARA12_BEST
#PHYS_PARA13_BEST
#PHYS_PARA14_BEST
#PHYS_PARA15_BEST
#PHYS_PARA16_BEST
#PHYS_PARA17_BEST
#PHYS_PARA18_BEST
#PHYS_PARA19_BEST
#PHYS_PARA20_BEST
#PHYS_PARA21_BEST
#PHYS_PARA22_BEST
#PHYS_PARA23_BEST
#PHYS_PARA24_BEST
#PHYS_PARA25_BEST
#PHYS_PARA26_BEST
#PHYS_PARA27_BEST
# based on ML analysis with MEDIAN,68p_INF,68p_SUP values
#PHYS_PARA1_MED
#PHYS_PARA2_MED
#PHYS_PARA3_MED
#PHYS_PARA4_MED
#PHYS_PARA5_MED
#PHYS_PARA6_MED
#PHYS_PARA7_MED
#PHYS_PARA8_MED
#PHYS_PARA9_MED
#PHYS_PARA10_MED
#PHYS_PARA11_MED
#PHYS_PARA12_MED
#PHYS_PARA13_MED
#PHYS_PARA14_MED
#PHYS_PARA15_MED
#PHYS_PARA16_MED
#PHYS_PARA17_MED
#PHYS_PARA18_MED
#PHYS_PARA19_MED
#PHYS_PARA20_MED
#PHYS_PARA21_MED
#PHYS_PARA22_MED
#PHYS_PARA23_MED
#PHYS_PARA24_MED
#PHYS_PARA25_MED
#PHYS_PARA26_MED
#PHYS_PARA27_MED
#PHYS_PARA1_INF
#PHYS_PARA2_INF
#PHYS_PARA3_INF
#PHYS_PARA4_INF
#PHYS_PARA5_INF
#PHYS_PARA6_INF
#PHYS_PARA7_INF
#PHYS_PARA8_INF
#PHYS_PARA9_INF
#PHYS_PARA10_INF
#PHYS_PARA11_INF
#PHYS_PARA12_INF
#PHYS_PARA13_INF
#PHYS_PARA14_INF
#PHYS_PARA15_INF
#PHYS_PARA16_INF
#PHYS_PARA17_INF
#PHYS_PARA18_INF
#PHYS_PARA19_INF
#PHYS_PARA20_INF
#PHYS_PARA21_INF
#PHYS_PARA22_INF
#PHYS_PARA23_INF
#PHYS_PARA24_INF
#PHYS_PARA25_INF
#PHYS_PARA26_INF
#PHYS_PARA27_INF
#PHYS_PARA1_SUP
#PHYS_PARA2_SUP
#PHYS_PARA3_SUP
#PHYS_PARA4_SUP
#PHYS_PARA5_SUP
#PHYS_PARA6_SUP
#PHYS_PARA7_SUP
#PHYS_PARA8_SUP
#PHYS_PARA9_SUP
#PHYS_PARA10_SUP
#PHYS_PARA11_SUP
#PHYS_PARA12_SUP
#PHYS_PARA13_SUP
#PHYS_PARA14_SUP
#PHYS_PARA15_SUP
#PHYS_PARA16_SUP
#PHYS_PARA17_SUP
#PHYS_PARA18_SUP
#PHYS_PARA19_SUP
#PHYS_PARA20_SUP
#PHYS_PARA21_SUP
#PHYS_PARA22_SUP
#PHYS_PARA23_SUP
#PHYS_PARA24_SUP
#PHYS_PARA25_SUP
#PHYS_PARA26_SUP
#PHYS_PARA27_SUP
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IDENT
Z_BEST
Z_BEST68_LOW
Z_BEST68_HIGH
Z_ML
#Z_ML68_LOW
#Z_ML68_HIGH
#Z_BEST90_LOW
#Z_BEST90_HIGH
#Z_BEST99_LOW
#Z_BEST99_HIGH
CHI_BEST
MOD_BEST
EXTLAW_BEST
EBV_BEST
#ZF_BEST
#MAG_ABS_BEST
PDZ_BEST
SCALE_BEST
DIST_MOD_BEST
NBAND_USED
#NBAND_ULIM
#
####### Z-2nd GALAXY ###########
Z_SEC
CHI_SEC
MOD_SEC
#AGE_SEC
#EBV_SEC
#ZF_SEC
#MAG_ABS_SEC
#PDZ_SEC
#SCALE_SEC
#
######## Z-Best QSO #############
Z_QSO
CHI_QSO
MOD_QSO
#MAG_ABS_QSO
#DIST_MOD_QSO
######## Best STAR #############
MOD_STAR
CHI_STAR
#
######## OBSERVED MAGNITUDES ####
#MAG_OBS()
#ERR_MAG_OBS()
######## MODEL MAGNITUDES FOR GALAXY ####
#MAG_MOD()
#
######## K-COR , ABSOLUTE MAG, FILTER CHOICE FOR GALAXY ##########
#K_COR()
#MAG_ABS()
#MABS_FILT()
#
######## K-COR , ABSOLUTE MAG. FOR QSO ##########
#K_COR_QSO()
#MAG_ABS_QSO()
#
####### PROBABILITY PER Z BINS ##
#PDZ()
#
####### INPUT INFO ##############
CONTEXT
ZSPEC
#STRING_INPUT
####### Far-IR PARAMETERS derived from FIR_LIB library ###########
#LUM_TIR_BEST
#LIB_FIR
#MOD_FIR
#CHI2_FIR
#FSCALE_FIR
#NBAND_FIR
#LUM_TIR_MED
#LUM_TIR_INF
#LUM_TIR_SUP
#MAG_MOD_FIR()
#MAG_ABS_FIR()
#K_COR_FIR()
######### PHYSICAL PARAMETERS derived from ZPHOTLIB library IF DEFINED ######
#AGE_BEST
#AGE_INF
#AGE_MED
#AGE_SUP
##
#LDUST_BEST
#LDUST_INF
#LDUST_MED
#LDUST_SUP
##
#MASS_BEST
#MASS_INF
#MASS_MED
#MASS_SUP
#
#SFR_BEST
#SFR_INF
#SFR_MED
#SFR_SUP
#
#SSFR_BEST
#SSFR_INF
#SSFR_MED
#SSFR_SUP
#
#LUM_NUV_BEST
#LUM_R_BEST
#LUM_K_BEST
######### PHYSICAL PARAMETERS derived from PHYS_LIB library
# best Chi^2 or median+/-68% of the ML distribution
# 1: Lg(Age[yr])
# 2: Lg(Luv[Lo]) 3: Lg(Lr[Lo]) 4: Lg(Lk[Lo])
# 5: Lg(Ldust [Lo])
# 6: Lg(Mass[Mo]) 7: Lg(SFR_1e8[Mo/yr]) 8: Lg(SFR_1e9[Mo/yr])
# 9: Lg(Gamma[Gyr]) 10: Metallicity
# 11: Tauv 12: mu
# 13: Lg(Age_weightRlight[yr]) 14: Lg(Age_weightMass[yr])
# 15: Lg(Age_tlastburst[yr])
# 16: Log(Frac_burst_1.e8[yr]) 17: Lg(Frac_burst_1e9[yr]) 18: Nb burst
# 19: Lg(SSFR_1e8 [yr-1]) 20: Lg(SSFR_1e9 [yr-1])
# 21: A(1500) [mag] 22: A(2300) [mag] 23: A(4500) [mag]
# 24: A(6000) [mag] 25: A(8500) [mag] 26: A(22000)[mag]
# 27: Lg(Ldust_hot[Lo])
#PHYS_CHI2_BEST
#PHYS_MOD_BEST
#PHYS_MAG_MOD()
#PHYS_MAG_ABS()
#PHYS_K_COR()
#PHYS_PARA1_BEST
#PHYS_PARA2_BEST
#PHYS_PARA3_BEST
#PHYS_PARA4_BEST
#PHYS_PARA5_BEST
#PHYS_PARA6_BEST
#PHYS_PARA7_BEST
#PHYS_PARA8_BEST
#PHYS_PARA9_BEST
#PHYS_PARA10_BEST
#PHYS_PARA11_BEST
#PHYS_PARA12_BEST
#PHYS_PARA13_BEST
#PHYS_PARA14_BEST
#PHYS_PARA15_BEST
#PHYS_PARA16_BEST
#PHYS_PARA17_BEST
#PHYS_PARA18_BEST
#PHYS_PARA19_BEST
#PHYS_PARA20_BEST
#PHYS_PARA21_BEST
#PHYS_PARA22_BEST
#PHYS_PARA23_BEST
#PHYS_PARA24_BEST
#PHYS_PARA25_BEST
#PHYS_PARA26_BEST
#PHYS_PARA27_BEST
# based on ML analysis with MEDIAN,68p_INF,68p_SUP values
#PHYS_PARA1_MED
#PHYS_PARA2_MED
#PHYS_PARA3_MED
#PHYS_PARA4_MED
#PHYS_PARA5_MED
#PHYS_PARA6_MED
#PHYS_PARA7_MED
#PHYS_PARA8_MED
#PHYS_PARA9_MED
#PHYS_PARA10_MED
#PHYS_PARA11_MED
#PHYS_PARA12_MED
#PHYS_PARA13_MED
#PHYS_PARA14_MED
#PHYS_PARA15_MED
#PHYS_PARA16_MED
#PHYS_PARA17_MED
#PHYS_PARA18_MED
#PHYS_PARA19_MED
#PHYS_PARA20_MED
#PHYS_PARA21_MED
#PHYS_PARA22_MED
#PHYS_PARA23_MED
#PHYS_PARA24_MED
#PHYS_PARA25_MED
#PHYS_PARA26_MED
#PHYS_PARA27_MED
#PHYS_PARA1_INF
#PHYS_PARA2_INF
#PHYS_PARA3_INF
#PHYS_PARA4_INF
#PHYS_PARA5_INF
#PHYS_PARA6_INF
#PHYS_PARA7_INF
#PHYS_PARA8_INF
#PHYS_PARA9_INF
#PHYS_PARA10_INF
#PHYS_PARA11_INF
#PHYS_PARA12_INF
#PHYS_PARA13_INF
#PHYS_PARA14_INF
#PHYS_PARA15_INF
#PHYS_PARA16_INF
#PHYS_PARA17_INF
#PHYS_PARA18_INF
#PHYS_PARA19_INF
#PHYS_PARA20_INF
#PHYS_PARA21_INF
#PHYS_PARA22_INF
#PHYS_PARA23_INF
#PHYS_PARA24_INF
#PHYS_PARA25_INF
#PHYS_PARA26_INF
#PHYS_PARA27_INF
#PHYS_PARA1_SUP
#PHYS_PARA2_SUP
#PHYS_PARA3_SUP
#PHYS_PARA4_SUP
#PHYS_PARA5_SUP
#PHYS_PARA6_SUP
#PHYS_PARA7_SUP
#PHYS_PARA8_SUP
#PHYS_PARA9_SUP
#PHYS_PARA10_SUP
#PHYS_PARA11_SUP
#PHYS_PARA12_SUP
#PHYS_PARA13_SUP
#PHYS_PARA14_SUP
#PHYS_PARA15_SUP
#PHYS_PARA16_SUP
#PHYS_PARA17_SUP
#PHYS_PARA18_SUP
#PHYS_PARA19_SUP
#PHYS_PARA20_SUP
#PHYS_PARA21_SUP
#PHYS_PARA22_SUP
#PHYS_PARA23_SUP
#PHYS_PARA24_SUP
#PHYS_PARA25_SUP
#PHYS_PARA26_SUP
#PHYS_PARA27_SUP
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##############################################################################
# CREATION OF LIBRARIES FROM SEDs List #
# $LEPHAREDIR/source/sedtolib -t (S/Q/G) -c $LEPHAREDIR/config/zphot.para #
# help : $LEPHAREDIR/source/sedtolib -h (or -help) #
##############################################################################
#
#------ STELLAR LIBRARY (ASCII SEDs)
STAR_SED $LEPHAREDIR/sed/STAR/STAR_MOD.list # STAR list (full path)
STAR_FSCALE 3.432E-09 # Arbitrary Flux Scale
STAR_LIB LIB_STAR # Bin. STAR LIBRARY ->
# $LEPHAREWORK/lib_bin
#
#------ QSO LIBRARY (ASCII SEDs)
QSO_SED $LEPHAREDIR/sed/QSO/QSO_MOD.list # QSO list (full path)
QSO_FSCALE 1 # Arbitrary Flux Scale
QSO_LIB LIB_QSO # Bin. QSO LIBRARY ->
# $LEPHAREWORK/lib_bin
#
#------ GALAXY LIBRARY (ASCII or BINARY SEDs)
GAL_SED $LEPHAREDIR/sed/GAL/COSMOS_SED/COSMOS_MOD.list # GAL list (full path)
GAL_FSCALE 1. # Arbitrary Flux Scale
GAL_LIB LIB_CWW # Bin. GAL LIBRARY ->
# $LEPHAREWORK/lib_bin
#SEL_AGE $LEPHAREDIR/sed/GAL/HYPERZ/AGE_GISSEL_ALL.dat # Age list(full path)
# (def=NONE)
AGE_RANGE 0.,13.e9 # Age Min-Max in yr
#
#############################################################################
# FILTERS #
# $LEPHAREDIR/source/filter -c $LEPHAREDIR/config/zphot.para #
# help: $LEPHAREDIR/source/filter -h (or -help) #
#############################################################################
# Filter number and context
# f275 f435 f606 f775 f814 f850lp f105 f125 f140 f160
# 1 2 3 4 5 6 7 8 9 10
# 1 2 4 8 16 32 64 128 256 512= 511
#
FILTER_LIST hst_candles/f275w.dat,hst_candles/f435w.dat,hst_candles/f606w.dat,hst_candles/f775w.dat,hst_candles/f814w.dat,hst_candles/f850lp.dat,hst_candles/f105w.dat,hst_candles/f125w.dat,hst_candles/f140w.dat,hst_candles/f160w.dat
# (in $LEPHAREDIR/filt/*)
TRANS_TYPE 0 # TRANSMISSION TYPE
# 0[-def]: Energy, 1: Nb of photons
FILTER_CALIB 0 # 0[-def]: fnu=ctt
# 1 : nu.fnu=ctt
# 2 : fnu=nu
# 3 : fnu=Black Body @ T=10000K
# 4 : for MIPS (leff with nu fnu=ctt and flux with BB @ 10000K
FILTER_FILE candles.filt # output name of filter's file ->
# $LEPHAREWORK/filt/
#
############################################################################
# THEORETICAL MAGNITUDES #
# $LEPHAREDIR/source/mag_star -c $LEPHAREDIR/config/zphot.para (star only)#
# help: $LEPHAREDIR/source/mag_star -h (or -help) #
# $LEPHAREDIR/source/mag_gal -t (Q or G) -c $LEPHAREDIR/config/zphot.para #
# (for gal. & QSO) #
# help: $LEPHAREDIR/source/mag_gal -h (or -help) #
############################################################################
#
#------- From STELLAR LIBRARY
STAR_LIB_IN LIB_STAR # Input STELLAR LIBRARY in $LEPHAREWORK/lib_bin/
STAR_LIB_OUT STAR_HDF # Output STELLAR MAGN -> $LEPHAREWORK/lib_mag/
#
#------- From QSO LIBRARY
QSO_LIB_IN LIB_QSO # Input QSO LIBRARY in $LEPHAREWORK/lib_bin/
QSO_LIB_OUT QSO_HDF # Output QSO MAGN -> $LEPHAREWORK/lib_mag/
#
#------- From GALAXY LIBRARY
GAL_LIB_IN LIB_CWW # Input GAL LIBRARY in $LEPHAREWORK/lib_bin/
GAL_LIB_OUT CWW_HDF # Output GAL LIBRARY -> $LEPHAREWORK/lib_mag/
#
#------- MAG + Z_STEP + EXTINCTION + COSMOLOGY
MAGTYPE AB # Magnitude type (AB or VEGA)
Z_STEP 0.04,3.,0.1 # dz, zmax, dzsup(if zmax>6)
COSMOLOGY 70,0.3,0.7 # H0,om0,lbd0 (if lb0>0->om0+lbd0=1)
MOD_EXTINC 13,23,23,31,23,31,23,31 # model range for extinction
EXTINC_LAW SMC_prevot.dat,SB_calzetti.dat,SB_calzetti_bump1.dat,SB_calzetti_bump2.dat # ext. law (in $LEPHAREDIR/ext/*)
EB_V 0.000,0.100,0.200,0.300,0.400,0.500 # E(B-V) (<50 values)
EM_LINES YES
# Z_FORM 8,7,6,5,4,3 # Zformation for each SED in GAL_LIB_IN
#
#------- ASCII OUTPUT FILES OPTION
LIB_ASCII NO # Writes output in ASCII
# in working directory
#
############################################################################
# PHOTOMETRIC REDSHIFTS #
# $LEPHAREDIR/source/zphot -c $LEPHAREDIR/config/zphot.para #
# help: $LEPHAREDIR/source/zphot -h (or -help) #
############################################################################
#
#
#
#------- Input Catalog Informations
CAT_IN $LEPHAREWORK/test1.in # Input catalog (full path)
INP_TYPE M # Input type (F:Flux or M:MAG)
CAT_MAG AB # Input Magnitude (AB or VEGA)
CAT_FMT MEME # MEME: (Mag,Err)i
# MMEE: (Mag)i,(Err)i
CAT_LINES -99,-99 # MIN and MAX RANGE of ROWS used in input cat [def:-99,-99]
CAT_TYPE LONG # Input Format (LONG,SHORT-def)
CAT_OUT $LEPHAREWORK/config/zphot_1.out # Output catalog (full path)
PARA_OUT $LEPHAREWORK/config/zphot_output.para # Ouput parameter (full path)
#
BD_SCALE 0 # Bands used for scaling
# (Sum 2^n; n=0->nbd-1, 0[-def]:all bands)
GLB_CONTEXT 0 # Overwrite Context (Sum 2^n; n=0->nbd-1,
# 0 : all bands used,
# -1[-def]: used context per object
# FORB_CONTEXT -1 # context for forbitten bands
ERR_SCALE 0.03,0.02,0.02,0.02,0.04 # errors per band added in quadrature
ERR_FACTOR 1.0 # error scaling factor 1.0 [-def]
#
#------- Theoretical libraries
ZPHOTLIB CWW_HDF #,STAR_HDF,QSO_HDF # Library used for Chi2 (max:3)
ADD_EMLINES YES
#
######## PHOTOMETRIC REDSHIFTS OPTIONS ###########
# FIR LIBRARY
FIR_LIB NONE
FIR_LMIN 7.0 # Lambda Min (micron) for FIR analysis
FIR_CONT -1
FIR_SCALE -1
FIR_FREESCALE YES # ALLOW FOR FREE SCALING
FIR_SUBSTELLAR NO
# PHYSICAL LIBRARY with Stochastic models from BC07
PHYS_LIB NONE
PHYS_CONT -1
PHYS_SCALE -1
PHYS_NMAX 100000
#
#------- Priors
# MASS_SCALE 6.,16. # Lg(Scaling) min,max [0,0-def]
MAG_ABS -10.,-26. # Mabs_min , Mabs_max [0,0-def]
MAG_REF 4 # Reference number for band used by Mag_abs
# ZFORM_MIN 5,5,5,5,5,5,3,1 # Min. Zformation per SED -> Age constraint
Z_RANGE 0.,99.99 # Z min-max used for the Galaxy library
EBV_RANGE 0.2,0.9 # E(B-V) MIN-MAX RANGE of E(B-V) used
# NZ_PRIOR 4,2,4 # I Band for prior on N(z)
#
#------- Fixed Z (need format LONG for input Cat)
ZFIX YES # fixed z and search best model [YES,NO-def]
#
#------- Parabolic interpolation for Zbest
Z_INTERP YES # redshift interpolation [YES,NO-def]
#
#------- Analysis of normalized ML(exp-(0.5*Chi^2)) curve
#------- Secondary peak analysis
DZ_WIN 0.5 # Window search for 2nd peaks [0->5;0.25-def]
MIN_THRES 0.1 # Lower threshold for 2nd peaks[0->1; 0.1-def]
#
#------- Probability (in %) per redshift intervals
# PROB_INTZ 0,0.5,0.5,1.,1.,1.5 # even number
#
######### ABSOLUTE MAGNITUDES COMPUTATION ###########
#
MABS_METHOD 1 # 0[-def] : obs->Ref
# 1 : best obs->Ref
# 2 : fixed obs->Ref
# 3 : mag from best SED
# 4 : Zbin
MABS_CONTEXT -1 # CONTEXT for Band used for MABS
MABS_REF 4 # 0[-def]: filter obs chosen for Mabs :
# ONLY USED IF MABS_METHOD=2
MABS_FILT 1,2,3,4 # Chosen filters per redshift bin (MABS_ZBIN)
# ONLY USED IF MABS_METHOD=4
MABS_ZBIN 0,0.5,1,1.5,2,3,3.5,4 # Redshift bins (even number)
# ONLY USED IF MABS_METHOD=4
######### OUTPUT SPECTRA ###########
#
SPEC_OUT YES # spectrum for each object? [YES,NO-def]
CHI2_OUT NO # output file with all values : z,mod,chi2,E(B-V),...
# BE CAREFUL can take a lot of space !!
######### OUTPUT PDZ ANALYSIS
PDZ_OUT NONE # pdz output file name [def-NONE]
# add automatically PDZ_OUT[.pdz/.mabsx/.mod/.zph]
PDZ_MABS_FILT 2,10,14 # MABS for REF FILTERS to be extracted
#
######### FAST MODE : color-space reduction #####
#
FAST_MODE NO # Fast computation [NO-def]
COL_NUM 3 # Number of colors used [3-def]
COL_SIGMA 3 # Enlarge of the obs. color-errors[3-def]
COL_SEL AND # Combination between used colors [AND/OR-def]
#
######### MAGNITUDE SHIFTS applied to libraries ######
#
# APPLY_SYSSHIFT 0. # Apply systematic shifts in each band
# used only if number of shifts matches
# with number of filters in the library
#
######### ADAPTIVE METHOD using Z spectro sample ###
#
AUTO_ADAPT NO # Adapting method with spectro [NO-def]
ADAPT_BAND 4,2,4 # Reference band, band1, band2 for color
ADAPT_LIM 18,22.0 # Mag limits for spectro in Ref band [18,21.5-def]
ADAPT_POLY 1 # Number of coef in polynom (max=4) [1-def]
ADAPT_METH 1 # Fit as a function of
# 1 : Color Model [1-def]
# 2 : Redshift
# 3 : Models
ADAPT_CONTEXT -1 # Context for bands used for training
# -1[-def] used context per object
ADAPT_ZBIN 0.01,6 # Redshift's interval used for training
# [0.001,6-Def]
ADAPT_MODBIN 1,1000 # Model's interval used for training
# [1,1000-Def]
ERROR_ADAPT NO # [YES,NO-def]
# Add error in quadrature according to
# the difference between observed
# and predicted apparent magnitudes
#
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# 345 0.00000e+00 0 1
# 132 0.00000e+00 0 2
# 172 0.00000e+00 0 3
# 85 0.00000e+00 0 4
# 116 0.00000e+00 0 5
# 101 0.00000e+00 0 6
# 205 0.00000e+00 0 7
# 86 0.00000e+00 0 8
# 104 0.00000e+00 0 9
# 131 0.00000e+00 0 10
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CONFIG_FILE /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//config/zphot_su.para
LIB_TYPE G
LIB_FMT A
GAL_SED /Users/zhangxin/Work/photoz/Lephare/lephare_dev/sed/GAL/COSMOS_SED/COSMOS_MOD.list
GAL_LIB /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//lib_bin/LIB_CWW.bin
GAL_WMAX 1762
GAL_FSCALE 0.100000E+01
SEL_AGE NONE
AGE_RANGE 0.000000E+00 0.130000E+11
NUMBER_SED 31
MOD_000001 1 1762 1 COSMOS_SED/Ell1_A_0.sed
MOD_000002 2 1762 1 COSMOS_SED/Ell2_A_0.sed
MOD_000003 3 1762 1 COSMOS_SED/Ell3_A_0.sed
MOD_000004 4 1762 1 COSMOS_SED/Ell4_A_0.sed
MOD_000005 5 1762 1 COSMOS_SED/Ell5_A_0.sed
MOD_000006 6 1762 1 COSMOS_SED/Ell6_A_0.sed
MOD_000007 7 1762 1 COSMOS_SED/Ell7_A_0.sed
MOD_000008 8 1762 1 COSMOS_SED/S0_A_0.sed
MOD_000009 9 1762 1 COSMOS_SED/Sa_A_0.sed
MOD_000010 10 1762 1 COSMOS_SED/Sa_A_1.sed
MOD_000011 11 1762 1 COSMOS_SED/Sb_A_0.sed
MOD_000012 12 1762 1 COSMOS_SED/Sb_A_1.sed
MOD_000013 13 1762 1 COSMOS_SED/Sc_A_0.sed
MOD_000014 14 1762 1 COSMOS_SED/Sc_A_1.sed
MOD_000015 15 1762 1 COSMOS_SED/Sc_A_2.sed
MOD_000016 16 1762 1 COSMOS_SED/Sd_A_0.sed
MOD_000017 17 1762 1 COSMOS_SED/Sd_A_1.sed
MOD_000018 18 1762 1 COSMOS_SED/Sd_A_2.sed
MOD_000019 19 1762 1 COSMOS_SED/Sdm_A_0.sed
MOD_000020 20 1762 1 COSMOS_SED/SB0_A_0.sed
MOD_000021 21 1762 1 COSMOS_SED/SB1_A_0.sed
MOD_000022 22 1762 1 COSMOS_SED/SB2_A_0.sed
MOD_000023 23 1762 1 COSMOS_SED/SB3_A_0.sed
MOD_000024 24 1762 1 COSMOS_SED/SB4_A_0.sed
MOD_000025 25 1762 1 COSMOS_SED/SB5_A_0.sed
MOD_000026 26 1762 1 COSMOS_SED/SB6_A_0.sed
MOD_000027 27 1762 1 COSMOS_SED/SB7_A_0.sed
MOD_000028 28 1762 1 COSMOS_SED/SB8_A_0.sed
MOD_000029 29 1762 1 COSMOS_SED/SB9_A_0.sed
MOD_000030 30 1762 1 COSMOS_SED/SB10_A_0.sed
MOD_000031 31 1762 1 COSMOS_SED/SB11_A_0.sed
CREATION_DATE Tue Jun 21 11:56:41 2022
NUMBER_ROWS 62
RECORD_LENGTH 14128
NUMBER_LBDA 1762
NUMBER_AGE 1
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1 1 -0.100000E+01 0.252529E+02 0.269553E+02 0.271096E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.145462E+01
2 1 -0.990000E+02 0.252529E+02 0.269553E+02 0.271096E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.145462E+01
3 2 -0.100000E+01 0.251921E+02 0.269854E+02 0.271880E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.147572E+01
4 2 -0.990000E+02 0.251921E+02 0.269854E+02 0.271880E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.147572E+01
5 3 -0.100000E+01 0.251392E+02 0.270052E+02 0.272356E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.150687E+01
6 3 -0.990000E+02 0.251392E+02 0.270052E+02 0.272356E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.150687E+01
7 4 -0.100000E+01 0.250623E+02 0.270317E+02 0.272986E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.155319E+01
8 4 -0.990000E+02 0.250623E+02 0.270317E+02 0.272986E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.155319E+01
9 5 -0.100000E+01 0.250108E+02 0.270525E+02 0.273503E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.158775E+01
10 5 -0.990000E+02 0.250108E+02 0.270525E+02 0.273503E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.158775E+01
11 6 -0.100000E+01 0.249192E+02 0.270821E+02 0.274045E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.165339E+01
12 6 -0.990000E+02 0.249192E+02 0.270821E+02 0.274045E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.165339E+01
13 7 -0.100000E+01 0.248958E+02 0.271114E+02 0.274674E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.172472E+01
14 7 -0.990000E+02 0.248958E+02 0.271114E+02 0.274674E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.172472E+01
15 8 -0.100000E+01 0.251638E+02 0.271349E+02 0.275663E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.181843E+01
16 8 -0.990000E+02 0.251638E+02 0.271349E+02 0.275663E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.181843E+01
17 9 -0.100000E+01 0.252943E+02 0.271098E+02 0.275273E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.175930E+01
18 9 -0.990000E+02 0.252943E+02 0.271098E+02 0.275273E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 -0.990000E+02 0.175930E+01
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CONFIG_FILE /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//config/zphot_su.para
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CONFIG_FILE /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//config/zphot_su.para
LIB_TYPE S
LIB_FMT A
STAR_SED /Users/zhangxin/Work/photoz/Lephare/lephare_dev/sed/STAR/STAR_MOD.list
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STAR_FSCALE 0.343200E-08
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CONFIG_FILE /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//config/zphot_su.para
LIB_TYPE GALAXY
LIB_NAME LIB_CWW
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FILTER_FILE candles.filt
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EXTINC_LAW SMC_prevot.dat SB_calzetti.dat SB_calzetti_bump1.dat SB_calzetti_bump2.dat
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EB_V 0.000 0.100 0.200 0.300 0.400 0.500
EM_LINES YES
CREATION_DATE Tue Jun 21 11:56:39 2022
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CONFIG_FILE /Users/zhangxin/Work/SED_PRJ/superSim/LePhare//config/zphot_su.para
LIB_TYPE QSO
LIB_NAME LIB_QSO
NUMBER_SED 28
NUMBER_ROWS 13148
RECORD_LENGTH 224
FILTER_FILE candles.filt
FILTERS 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00 0.00000e+00
MAG_TYPE AB
AB_COR 1.572 -0.080 0.091 0.403 0.436 0.537 0.651 0.908 1.084 1.270
FLUX_COR 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000 1.000
Z_STEP 0.040 3.000 0.100
COSMOLOGY 70.000 0.300 0.700
EXTINC_LAW SMC_prevot.dat SB_calzetti.dat SB_calzetti_bump1.dat SB_calzetti_bump2.dat
MOD_EXTINC 13 23 23 31 23 31 23 31
EB_V 0.000 0.100 0.200 0.300 0.400 0.500
EM_LINES NO
CREATION_DATE Tue Jun 21 11:56:19 2022
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