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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 
#   f300 f450 f606 f814 J  H  K 
#   1    2    3    4    5  6  7
#   1    2    4    8   16  32 64 = 127 
#
FILTER_LIST tmp/f300.pb,tmp/f450.pb,tmp/f606.pb,tmp/f814.pb,tmp/Jbb.pb,tmp/H.pb,tmp/K.pb
					# (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	HDF.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 	0,0		     # model range for extinction 
EXTINC_LAW	calzetti.dat	     # ext. law (in  $LEPHAREDIR/ext/*)
EB_V            0.,0.05,0.1,0.2,0.3  # E(B-V) (<50 values)
EM_LINES        NO  
# 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       $LEPHAREDIR/test/hdfn_lanzetta.in  # Input catalog  (full path) 
INP_TYPE     F		          # 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    1,100000             #  MIN and MAX RANGE of ROWS used in input cat [def:-99,-99]
CAT_TYPE     LONG	          # Input Format    (LONG,SHORT-def)
CAT_OUT	     $LEPHAREDIR/test/zphot.out	# Output catalog (full path) 
PARA_OUT     $LEPHAREDIR/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  0.03,0.02,0.02,0.02,0.04,0.04,0.04  # errors per band added in quadrature
ERR_FACTOR  1.5                    # error scaling factor 1.0 [-def] 
#
#-------    Theoretical libraries  
ZPHOTLIB    CWW_HDF,STAR_HDF,QSO_HDF    # Library used for Chi2 (max:3)
ADD_EMLINES  NO 
#
########    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		NO		 # 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	NO	 	 # 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 
#