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Commit c29dd74f authored by ILBERT Olivier's avatar ILBERT Olivier
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Improve the documentation, and clean few SED directories

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config/COSMOS.para 0 → 100644
View file @ c29dd74f
##############################################################################################
########### CREATION OF LIBRARIES FROM SEDs List #############
########### Run : $ZPHOTDIR/source/sedtolib -t (S/Q/G) -c zphot.para #############
##############################################################################################
#
#------------------- STELLAR LIBRARY (ASCII SEDs) ---------------------------
STAR_SED STAR_SWIRE.list # STAR list (full path)
STAR_LIB LIB_STAR # Binary STAR LIBRARY (-> $ZPHOTWORK/lib_bin/*)
STAR_FSCALE 3.432E-09 # Arbitrary Flux Scale
#
#------------------- QSO LIBRARY (ASCII SEDs) ---------------------------
QSO_SED AGN_LONSDALE.list # QSO list (full path)
QSO_LIB LIB_QSO # Binary QSO LIBRARY (-> $ZPHOTWORK/lib_bin/*)
QSO_FSCALE 1. # Arbitrary Flux Scale
#
#------------------- GALAXY LIBRARY (ASCII or BINARY SEDs) ---------------------------
GAL_SED CE_MOD.list # GALAXMuzzin09_SEDY list (full path)
GAL_LIB LIB_CE # Binary GAL LIBRARY (-> $ZPHOTWORK/lib_bin/*)
GAL_FSCALE 1. # Arbitrary Flux Scale
#SEL_AGE /data/zphot_vers25_03_03/sed/GAL/HYPERZ/AGE_GISSEL_HZ.dat # List of Age for GISSEL(full path)
AGE_RANGE 0.,15.e9 # Age Min-Max in yr
#
##############################################################################################
########### FILTERS #############
########### Run : $ZPHOTDIR/source/filter -c zphot.para #############
##############################################################################################
#
FILTER_REP $LEPHAREDIR/filt # Repository in which the filters are stored
FILTER_LIST cosmos/u_cfht.lowres,cosmos/B_subaru.lowres,cosmos/V_subaru.lowres,cosmos/r_subaru.lowres,cosmos/i_subaru.lowres,cosmos/suprime_FDCCD_z.res,hsc/yHSC.pb,vista/Y.lowres,vista/J.lowres,vista/H.lowres,vista/K.lowres,cosmos/H_wircam.lowres,cosmos/K_wircam.lowres,cosmos/IB427.lowres,cosmos/IB464.lowres,cosmos/IB484.lowres,cosmos/IB505.lowres,cosmos/IB527.lowres,cosmos/IB574.lowres,cosmos/IB624.lowres,cosmos/IB679.lowres,cosmos/IB709.lowres,cosmos/IB738.lowres,cosmos/IB767.lowres,cosmos/IB827.lowres,cosmos/NB711.lowres,cosmos/NB816.lowres,cosmos/irac_ch1.lowres,cosmos/irac_ch2.lowres,cosmos/irac_ch3.lowres,cosmos/irac_ch4.lowres,galex/NUV.lowres,galex/F1600.pb,cfht/u_megaprime_sagem.res,cfht/g_megaprime_sagem.res,cfht/r_megaprime_sagem.res,cfht/i_megaprime_sagem.res,cfht/iMegaNew.fil,cfht/z_megaprime_sagem.res
TRANS_TYPE 1 # TRANSMISSION TYPE
# 0[-def]: Energy, 1: Nb of photons
FILTER_CALIB 0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1,1,1,1,0,0,0,0,0,0,0,0 # 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 filter_cosmos # name of file with filters (-> $ZPHOTWORK/filt/)
#
##############################################################################################
########### THEORETICAL MAGNITUDES #############
########### Run : $ZPHOTDIR/source/mag_star -c zphot.para (star only) #######
########### Run : $ZPHOTDIR/source/mag_gal -t (Q or G) -c zphot.para (Gal. & QSO) #######
##############################################################################################
#
#------------------- From STELLAR LIBRARY ------------------------------
STAR_LIB_IN LIB_STAR # Input STELLAR LIBRARY (in $ZPHOTWORK/lib_bin/*)
STAR_LIB_OUT STAR_COSMOS # Output STELLAR MAGN. (-> $ZPHOTWORK/lib_mag/*)
#
#------------------- From QSO LIBRARY ------------------------------
QSO_LIB_IN LIB_QSO # Input QSO LIBRARY (in $ZPHOTWORK/lib_bin/*)
QSO_LIB_OUT QSO_COSMOS # Output QSO MAGN. (-> $ZPHOTWORK/lib_
#
#------------------- From GALAXY LIBRARY ------------------------------
GAL_LIB_IN LIB_CE # Input GALAXY LIBRARY (in $ZPHOTWORK/lib_bin/*)
GAL_LIB_OUT CE_COSMOS # Output GALAXY LIBRARY (-> $ZPHOTWORK/lib_mag/*)
#
#------------------ MAG + Z_STEP + COSMO + EXTINCTION -----------------------------
MAGTYPE AB # Magnitude type (AB or VEGA)
ZGRID_TYPE 0 # Define the kind of redshift grid (0: linear ; 1: dz*(1+z))
Z_STEP 0.01,0.,6. # dz, zmin, zmax
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 SB_calzetti.dat # ext. law (in $ZPHOTDIR/ext/*)
EB_V 0.,0.05,0.1,0.15,0.2,0.25,0.3,0.35,0.4,0.5 # E(B-V) (<50 values)
EM_LINES EMP_UV # [NO/EMP_UV/EMP_SFR/PHYS] choice between emission line prescription
EM_DISPERSION 0.5,0.75,1.,1.5,2. # Dispersion allowed in the emission line flux factor
#
#------------------ ASCII OUTPUT FILES OPTION -------------------------------
LIB_ASCII NO # Writing Output in ASCII file (-> working directory)
#
##############################################################################################
########### PHOTOMETRIC REDSHIFTS #############
########### Run : $ZPHOTDIR/source/zphot -c zphot.para #############
##############################################################################################
#
#------------------ Input Catalog Informations -------------------------------
CAT_IN bidon # 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 0,1000000000 # MIN and MAX RANGE of ROWS used in input cat [def:-99,-99]
CAT_TYPE LONG # Input Format (LONG,SHORT-def)
BD_SCALE 0 # Bands used for scaling (Sum 2^n; n=0->nbd-1, 0->all bands)
GLB_CONTEXT 0 # Overwrite Context (Sum 2^n; n=0->nbd-1, 0->all bands, -1[-def] used context per object)
FORB_CONTEXT -1 # Not consider these filters in the fit (Sum 2^n; n=0->nbd-1)
ERR_SCALE 0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.05,0.05,0.05,0.05,0.05,0.05,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.02,0.05,0.1,0.2,0.2,0.1,0.3,0.02,0.02,0.02,0.02,0.02,0.02 # Systematic errors per band
ERR_FACTOR 1.5
#
#------------------ Theoretical libraries --------------------------------
ZPHOTLIB CE_COSMOS,STAR_COSMOS,QSO_COSMOS # Library used for Chi2 (max:3)
ADD_EMLINES 0,100 # range of model in which to apply emission lines
#
#------------------ Output catalog Name ---------------------------------
CAT_OUT zphot.out # Output catalog (-> working directory)
PARA_OUT output.para # Ouput parameters (full path)
#
################# 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 -24,-5 # Mabs_min , Mabs_max [0,0-def]
MAG_ABS_AGN -30,-10 # Mabs_min , Mabs_max for AGN [0,0-def]
MAG_REF 2 # Reference number for band used by Mag_abs
#ZFORM_MIN 1,5,5,5,5,5,3,1 # 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 4,5 # I Band for prior on N(z), the second number is the band to be used if the first is missing.
#
#------------------ 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
#
Z_METHOD BEST # BEST/ML absolute magnitude, .spec, scaling will be given at this redshift
#------------------ Normalized ML(exp-(0.5*Chi^2)) curve analysis -------------------
#------- Secondary peak analysis
DZ_WIN 0.3 # Window search for 2nd peaks [0->5; 0.25-def]
MIN_THRES 0.02 # Lower theshold for 2nd peaks [0->1; 0.1-def]
#
#------- Probability (in %) per redshift intervals --------------------
#PROB_INTZ 0.01,0.1,0.1,0.2,0.2,0.3,0.3,0.4,0.4,0.5,0.5,0.6,0.6,0.7,0.7,0.8,0.8,0.9,0.9,1.,1.,1.1,1.1,1.3,1.3,1.5,1.5,2.,2.,3.,3.,4.,4.,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 2281702809
MABS_REF 11 # 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
RF_COLORS 32,4,4,13
ADDITIONAL_MAG none # name of file with filters (-> $ZPHOTWORK/filt/). Predicted mag and abs mag in additional filters.
######### Z MAX #####################################
LIMITS_ZBIN 0,99 # Redshifts used to split in N bins, separated by a coma. Need N+1 values (start with the minimum redshift).
LIMITS_MAPP_REF 1 # Band in which the absolute magnitude is computed
LIMITS_MAPP_SEL 1 # Give the selection band in each redshift bin. Need 1 or N values.
LIMITS_MAPP_CUT 90 # Magnitude cut used in each redshift bin. Need 1 or N values.
######### 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 5 # Reference band, band1, band2 for color
ADAPT_LIM 1.5,20.5 # Mag limits for spectro in Ref band [18,21.5-def]
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
#
config/output.para 0 → 100644
View file @ c29dd74f
# BASIC PHOTOZ INFORMATION
IDENT
Z_BEST
#Z_BEST68_LOW
#Z_BEST68_HIGH
#Z_BEST90_LOW
#Z_BEST90_HIGH
#Z_BEST99_LOW
#Z_BEST99_HIGH
Z_ML
Z_ML68_LOW
Z_ML68_HIGH
#Z_ML90_LOW
#Z_ML90_HIGH
#Z_ML99_LOW
#Z_ML99_HIGH
# INFORMATIONS ON THE BEST FIT TEMPLATE
CHI_BEST
MOD_BEST
EXTLAW_BEST
EBV_BEST
PDZ_BEST
SCALE_BEST
NBAND_USED
NBAND_ULIM
####### Z- 2nd solution - GALAXY ###########
Z_SEC
CHI_SEC
MOD_SEC
#AGE_SEC
#EBV_SEC
#EXTLAW_SEC
#PDZ_SEC
#SCALE_SEC
######## Best fit STAR #############
CHI_STAR
MOD_STAR
######## QSO #############
CHI_QSO
Z_QSO
MOD_QSO
#Z_ML_QSO
#Z_ML68_LOW_QSO
#Z_ML68_HIGH_QSO
######## MODEL MAGNITUDES FOR GALAXY ####
######## K-COR , ABSOLUTE MAG, FILTER CHOICE FOR GALAXY ##########
#MAG_MOD()
#MAG_PRED()
#K_COR()
#MAG_ABS()
#MABS_FILT()
#EMAG_ABS()
#ABSMAG_PRED()
# PHYSICAL PARAMETER FROM THE BEST FIT TEMPLATE (AT MINIMUM CHI2)
#EBV_BEST
#EBV_MED
#EBV_INF
#EBV_SUP
#AGE_BEST
#AGE_MED
#AGE_INF
#AGE_SUP
#LDUST_BEST
#LDUST_MED
#LDUST_INF
#LDUST_SUP
#MASS_BEST
#MASS_MED
#MASS_INF
#MASS_SUP
#SFR_BEST
#SFR_MED
#SFR_INF
#SFR_SUP
#SSFR_BEST
#SSFR_MED
#SSFR_INF
#SSFR_SUP
#COL1_MED
#COL1_INF
#COL1_SUP
#COL2_MED
#COL2_INF
#COL2_SUP
#MREF_MED
#MREF_INF
#MREF_SUP
#LUM_NUV_BEST
#LUM_R_BEST
#LUM_K_BEST
## LUM TIR FROM FIR FIT
#LUM_TIR_BEST
#LUM_TIR_MED
#LUM_TIR_INF
#LUM_TIR_SUP
######## LIMITS FROM MAG CUT ####
#LIMITS_ZMAX
#LIMITS_MFAINT
####### INPUT INFO ##############
#CONTEXT
ZSPEC
MAG_OBS()
ERR_MAG_OBS()
STRING_INPUT
config/output.para~ 0 → 100644
View file @ c29dd74f
// GALAXY
stout.unsetf(ios::fixed); //There is a problem with Z_BEST: for rare pathological galaxies is =-1.e9
if((outkeywords[k]).compare("Z_BEST") == 0)stout << setw(16) << setprecision(4) << zmin[0] << " ";
stout.setf(ios::fixed, ios::floatfield); stout.precision(4); //set float format and the n. of decimal digits
if((outkeywords[k]).compare("Z_BEST68_LOW") == 0)stout << setw(12) << z68[0] << " ";
if((outkeywords[k]).compare("Z_BEST68_HIGH") == 0)stout << setw(12) << z68[1] << " ";
if((outkeywords[k]).compare("Z_BEST90_LOW") == 0)stout << setw(12) << z90[0] << " ";
if((outkeywords[k]).compare("Z_BEST90_HIGH") == 0)stout << setw(12) << z90[1] << " ";
if((outkeywords[k]).compare("Z_BEST99_LOW") == 0)stout << setw(12) << z99[0] << " ";
if((outkeywords[k]).compare("Z_BEST99_HIGH") == 0)stout << setw(12) << z99[1] << " ";
if((outkeywords[k]).compare("Z_ML") == 0)stout << setw(12) << zml << " ";
if((outkeywords[k]).compare("Z_ML68_LOW") == 0)stout << setw(12) << zml68[0] << " ";
if((outkeywords[k]).compare("Z_ML68_HIGH") == 0)stout << setw(12) << zml68[1] << " ";
if((outkeywords[k]).compare("Z_ML90_LOW") == 0)stout << setw(12) << zml90[0] << " ";
if((outkeywords[k]).compare("Z_ML90_HIGH") == 0)stout << setw(12) << zml90[1] << " ";
if((outkeywords[k]).compare("Z_ML99_LOW") == 0)stout << setw(12) << zml99[0] << " ";
if((outkeywords[k]).compare("Z_ML99_HIGH") == 0)stout << setw(12) << zml99[1] << " ";
// Best fit values
double massBest = -99.9;
double sfrBest = -99.9;
double ssfrBest = -99.9;
double ldustBest= -99.9;
double lirBest = -99.9;
double ageBest = -99.9;
double ebvBest = -99.9;
double extlBest = -99.9;
double luvBest = -99.9;
double loptBest = -99.9;
double lnirBest = -99.9;
if(indmin[0]>=0){
massBest =log10((fulllib[indmin[0]])->mass * dmmin[0]);
sfrBest =log10((fulllib[indmin[0]])->sfr * dmmin[0]);
ssfrBest =log10((fulllib[indmin[0]])->sfr / (fulllib[indmin[0]])->mass);
ldustBest=(fulllib[indmin[0]])->ltir + log10(dmmin[0]);
ageBest =(fulllib[indmin[0]])->age ;
ebvBest =(fulllib[indmin[0]])->ebv;
extlBest =(fulllib[indmin[0]])->extlawId;
luvBest =(fulllib[indmin[0]])->luv + log10(3.e18*400/pow(2300,2)) -log10(Lsol)+log10(dmmin[0]);
loptBest =(fulllib[indmin[0]])->lopt+ log10(3.e18*1000/pow(6000,2)) -log10(Lsol)+log10(dmmin[0]);
lnirBest =(fulllib[indmin[0]])->lnir+ log10(3.e18*2000/pow(22000,2))-log10(Lsol)+log10(dmmin[0]);
}
if(indminIR>=0)lirBest =(fulllibIR[indminIR])->ltir + log10(dmminIR);
//Integer
stout.precision(0); // in fixed format, number of decimal digits in the output
if((outkeywords[k]).compare("MOD_BEST") == 0) stout << setw(6) << std::fixed << imasmin[0] << " " ;
if((outkeywords[k]).compare("EXTLAW_BEST") == 0) stout << setw(6) << std::fixed << extlBest << " ";
//Float
stout.setf(ios::fixed, ios::floatfield);
if((outkeywords[k]).compare("EBV_BEST") == 0) stout << setw(12) << setprecision(3) << ebvBest << " ";
if((outkeywords[k]).compare("MASS_BEST") == 0) stout << setw(12) << setprecision(5) << massBest << " ";
if((outkeywords[k]).compare("LDUST_BEST") == 0) stout << setw(12) << setprecision(3) << ldustBest << " ";
if((outkeywords[k]).compare("LUM_TIR_BEST")== 0) stout << setw(12) << setprecision(3) << lirBest << " ";
if((outkeywords[k]).compare("LUM_NUV_BEST") == 0)stout << setw(12) << setprecision(3) << luvBest << " ";
if((outkeywords[k]).compare("LUM_R_BEST") == 0) stout << setw(12) << setprecision(3) << loptBest << " ";
if((outkeywords[k]).compare("LUM_K_BEST") == 0) stout << setw(12) << setprecision(3) << lnirBest << " ";
//Scientific
stout.setf(ios::scientific, ios::floatfield);
//note: PDZ_BEST has to be fixed
if((outkeywords[k]).compare("PDZ_BEST") == 0) stout << setw(14) << setprecision(5) << 99. << " ";
if((outkeywords[k]).compare("CHI_BEST") == 0) stout << setw(14) << setprecision(5) << chimin[0]<< " ";
if((outkeywords[k]).compare("SCALE_BEST") == 0) stout << setw(14) << setprecision(5) << dmmin[0] << " ";
if((outkeywords[k]).compare("AGE_BEST") == 0) stout << setw(12) << setprecision(3) << ageBest << " " ;
if((outkeywords[k]).compare("SFR_BEST") == 0) stout << setw(12) << setprecision(3) << sfrBest << " ";
if((outkeywords[k]).compare("SSFR_BEST") == 0) stout << setw(12) << setprecision(3) << ssfrBest << " ";
/*
* The following parameters are not implemented yet:
* PDZ()
*/
// GENERAL
if((outkeywords[k]).compare("STRING_INPUT") == 0)stout << " " << str_inp << " " ; //string-like
stout.setf(ios::fixed); stout.precision(0); //Integer:
if((outkeywords[k]).compare("CONTEXT") == 0)stout << setw(16) << cont << " ";
if((outkeywords[k]).compare("NBAND_USED") == 0)stout << setw(5) << nbused << " ";
if((outkeywords[k]).compare("NBAND_ULIM") == 0)stout << setw(3) << nbul << " ";
stout.setf(ios::fixed, ios::floatfield); //Float:
if((outkeywords[k]).compare("ZSPEC") == 0)stout << setw(14) << setprecision(5) << zs << " " ;
if((outkeywords[k]).compare("MAG_OBS()") == 0){for (size_t l=0; l<mab.size(); l++)stout << setw(10) << setprecision(3) << mab[l] << " ";}
if((outkeywords[k]).compare("ERR_MAG_OBS()") == 0){for (size_t l=0; l<msab.size(); l++)stout << setw(10) << setprecision(3) << msab[l] << " ";}
if((outkeywords[k]).compare("MAG_MOD()") == 0){for (size_t l=0; l<magm.size(); l++)stout << setw(10) << setprecision(3) << magm[l] << " ";}
// QSO and STARS
stout.setf(ios::fixed); stout.precision(0); //Integer:
if((outkeywords[k]).compare("MOD_QSO") == 0)stout << setw(12) << imasmin[1] << " ";
if((outkeywords[k]).compare("MOD_STAR") == 0)stout << setw(12) << imasmin[2] << " ";
stout.setf(ios::fixed, ios::floatfield); stout.precision(4); //Float:
if((outkeywords[k]).compare("Z_QSO") == 0)stout << setw(12) << zmin[1] << " " ;
if((outkeywords[k]).compare("Z_ML_QSO") == 0)stout << setw(12) << zqml << " ";
if((outkeywords[k]).compare("Z_ML68_LOW_QSO") == 0)stout << setw(12) << zqml68[0] << " ";
if((outkeywords[k]).compare("Z_ML68_HIGH_QSO") == 0)stout << setw(12) << zqml68[1] << " ";
stout.setf(ios::scientific, ios::floatfield); stout.precision(5); //Scientific:
if((outkeywords[k]).compare("CHI_QSO") == 0)stout << setw(14) << chimin[1] << " ";
if((outkeywords[k]).compare("CHI_STAR") == 0)stout << setw(14) << chimin[2] << " ";
// SECONDARY GALAXY PEAK
stout.setf(ios::fixed); stout.precision(0); //Integer:
if((outkeywords[k]).compare("MOD_SEC") == 0)stout << setw(12) << zsecMod << " ";
if((outkeywords[k]).compare("EXTLAW_SEC")== 0)stout << setw(12) << zsecExtlaw<< " ";
stout.setf(ios::fixed, ios::floatfield); stout.precision(4); //Float:
if((outkeywords[k]).compare("Z_SEC") == 0)stout << setw(12) << zsec << " ";
if((outkeywords[k]).compare("EBV_SEC") == 0)stout << setw(12) << zsecEbv<< " ";
stout.setf(ios::scientific, ios::floatfield); stout.precision(5); //Scientific:
if((outkeywords[k]).compare("PDZ_SEC") == 0)stout << setw(14) << zsecProb << " " ;
if((outkeywords[k]).compare("CHI_SEC") == 0)stout << setw(14) << zsecChi2 << " " ;
if((outkeywords[k]).compare("SCALE_SEC") == 0)stout << setw(14) << zsecScale << " " ;
if((outkeywords[k]).compare("AGE_SEC") == 0)stout << setw(14) << zsecAge << " " ;
// PHYSICAL PARAMETERS
stout.setf(ios::fixed, ios::floatfield); stout.precision(5); //Float:
if((outkeywords[k]).compare("AGE_MED") == 0)stout << setw(12) << ageml << " " ;
if((outkeywords[k]).compare("AGE_INF") == 0)stout << setw(12) << ageml68[0] << " ";
if((outkeywords[k]).compare("AGE_SUP") == 0)stout << setw(12) << ageml68[1] << " ";
if((outkeywords[k]).compare("LDUST_MED") == 0)stout << setw(12) << Ldustml << " " ;
if((outkeywords[k]).compare("LDUST_INF") == 0)stout << setw(12) << Ldustml68[0] << " ";
if((outkeywords[k]).compare("LDUST_SUP") == 0)stout << setw(12) << Ldustml68[1] << " ";
if((outkeywords[k]).compare("LUM_TIR_MED") == 0)stout << setw(12) << LIRml << " " ;
if((outkeywords[k]).compare("LUM_TIR_INF") == 0)stout << setw(12) << LIRml68[0] << " ";
if((outkeywords[k]).compare("LUM_TIR_SUP") == 0)stout << setw(12) << LIRml68[1] << " ";
if((outkeywords[k]).compare("MASS_MED") == 0)stout << setw(12) << massml << " ";
if((outkeywords[k]).compare("MASS_INF") == 0)stout << setw(12) << massml68[0] << " ";
if((outkeywords[k]).compare("MASS_SUP") == 0)stout << setw(12) << massml68[1] << " ";
if((outkeywords[k]).compare("SFR_MED") == 0)stout << setw(12) << SFRml << " ";
if((outkeywords[k]).compare("SFR_INF") == 0)stout << setw(12) << SFRml68[0] << " ";
if((outkeywords[k]).compare("SFR_SUP") == 0)stout << setw(12) << SFRml68[1] << " ";
if((outkeywords[k]).compare("SSFR_MED") == 0)stout << setw(12) << sSFRml << " ";
if((outkeywords[k]).compare("SSFR_INF") == 0)stout << setw(12) << sSFRml68[0] << " ";
if((outkeywords[k]).compare("SSFR_SUP") == 0)stout << setw(12) << sSFRml68[1] << " ";
if((outkeywords[k]).compare("COL1_MED") == 0)stout << setw(12) << col1ml << " ";
if((outkeywords[k]).compare("COL1_INF") == 0)stout << setw(12) << col1ml68[0] << " ";
if((outkeywords[k]).compare("COL1_SUP") == 0)stout << setw(12) << col1ml68[1] << " ";
if((outkeywords[k]).compare("COL2_MED") == 0)stout << setw(12) << col2ml << " ";
if((outkeywords[k]).compare("COL2_INF") == 0)stout << setw(12) << col2ml68[0] << " ";
if((outkeywords[k]).compare("COL2_SUP") == 0)stout << setw(12) << col2ml68[1] << " ";
if((outkeywords[k]).compare("EBV_MED") == 0)stout << setw(12) << ebvml << " ";
if((outkeywords[k]).compare("EBV_INF") == 0)stout << setw(12) << ebvml68[0] << " ";
if((outkeywords[k]).compare("EBV_SUP") == 0)stout << setw(12) << ebvml68[1] << " ";
if((outkeywords[k]).compare("MREF_MED") == 0)stout << setw(12) << Mrefml << " ";
if((outkeywords[k]).compare("MREF_INF") == 0)stout << setw(12) << Mrefml68[0] << " ";
if((outkeywords[k]).compare("MREF_SUP") == 0)stout << setw(12) << Mrefml68[1] << " ";
// ABSOLUTE MAGNITUDES
stout.setf(ios::fixed); stout.precision(0); //Integer:
if((outkeywords[k]).compare("MABS_FILT()") == 0){for (size_t l=0; l<absfilt.size(); l++)stout << setw(4) << absfilt[l] << " " ;}
stout.setf(ios::fixed, ios::floatfield); stout.precision(3); //Float:
if((outkeywords[k]).compare("K_COR()") == 0){for (size_t l=0; l<kap.size(); l++)stout << setw(13) << setprecision(5) << kap[l] << " " ;}
if((outkeywords[k]).compare("MAG_ABS()") == 0){for (size_t l=0; l<mabs.size(); l++)stout << setw(12) << setprecision(5) << mabs[l] << " ";}
if((outkeywords[k]).compare("EMAG_ABS()") == 0){for (size_t l=0; l<emabs.size(); l++)stout << setw(13) << setprecision(5) << emabs[l] << " ";}
// PREDICTED MAGNITUDES IN ADDITIONAL FILTERS
stout.setf(ios::scientific, ios::floatfield); stout.precision(5);
if((outkeywords[k]).compare("MAG_PRED()") == 0){for (size_t l=0; l<magPred.size(); l++)stout << setw(15) << magPred[l] << " " ;}
if((outkeywords[k]).compare("ABSMAG_PRED()") == 0){for (size_t l=0; l<absmagPred.size(); l++)stout << setw(15) << absmagPred[l] << " " ;}
// EMISSION LINES
stout.setf(ios::scientific, ios::floatfield); stout.precision(5);
if((outkeywords[k]).compare("EM_FLUX_LYA") == 0) stout << setw(15) << setprecision(5) << flux_em[0] << " " ;
if((outkeywords[k]).compare("EM_FLUX_OII") == 0) stout << setw(15) << setprecision(5) << flux_em[1] << " ";
if((outkeywords[k]).compare("EM_FLUX_HB") == 0) stout << setw(15) << setprecision(5) << flux_em[2] << " ";
if((outkeywords[k]).compare("EM_FLUX_OIIIA") == 0) stout << setw(15) << setprecision(5) << flux_em[3] << " " ;
if((outkeywords[k]).compare("EM_FLUX_OIIIB") == 0) stout << setw(15) << setprecision(5) << flux_em[4] << " " ;
if((outkeywords[k]).compare("EM_FLUX_HA") == 0) stout << setw(15) << setprecision(5) << flux_em[5] << " " ;
if((outkeywords[k]).compare("EM_FLUX_SIIIA") == 0) stout << setw(15) << setprecision(5) << flux_em[6] << " " ;
if((outkeywords[k]).compare("EM_FLUX_SIIIB") == 0) stout << setw(15) << setprecision(5) << flux_em[7] << " " ;
if((outkeywords[k]).compare("EM_EW_LYA") == 0) stout << setw(15) << setprecision(5) << EW_em[0] << " " ;
if((outkeywords[k]).compare("EM_EW_OII") == 0) stout << setw(15) << setprecision(5) << EW_em[1] << " " ;
if((outkeywords[k]).compare("EM_EW_HB") == 0) stout << setw(15) << setprecision(5) << EW_em[2] << " " ;
if((outkeywords[k]).compare("EM_EW_OIIIA") == 0) stout << setw(15) << setprecision(5) << EW_em[3] << " " ;
if((outkeywords[k]).compare("EM_EW_OIIIB") == 0) stout << setw(15) << setprecision(5) << EW_em[4] << " " ;
if((outkeywords[k]).compare("EM_EW_HA") == 0) stout << setw(15) << setprecision(5) << EW_em[5] << " " ;
if((outkeywords[k]).compare("EM_EW_SIIIA") == 0) stout << setw(15) << setprecision(5) << EW_em[6] << " " ;
if((outkeywords[k]).compare("EM_EW_SIIIB") == 0) stout << setw(15) << setprecision(5) << EW_em[7] << " " ;
// LIMITS FOR VMAX
stout.setf(ios::fixed, ios::floatfield); stout.precision(4); //Float:
if((outkeywords[k]).compare("LIMITS_ZMAX") == 0)stout << setw(12) << limits_zmax << " " ;
if((outkeywords[k]).compare("LIMITS_MFAINT") == 0)stout << setw(12) << limits_Mfaint << " " ;
\ No newline at end of file
sed/GAL/CFHTLS_SED/.smhist 0 → 100644
View file @ c29dd74f
macro read plot_sed.sm
plot 0 2.9 4 30 35
macro read plot_sed.sm
plot 0 2.9 4 30 35
macro read plot_sed.sm
plot 0 2.9 4 30 35
macro read plot_sed.sm
plot 0 2.9 4 0 35
macro read plot_sed.sm
plot 0 2.9 4 0 35
plot 0 2.9 4 0 10
plot 0 2.9 4 -5 10
macro read plot_sed.sm
plot 0 2.9 4 -1 3
plot 0 2.9 5 -1 3
plot 0 2.9 4.3 -1 3
plot 0.8 2.9 4.3 -1 3
macro read plot_sed.sm
plot 0.8 2.9 4.3 -1 3
plot 0. 2.9 4.3 -1 3
plot 0. 2.9 40.3 -1 3
plot 0. 2.9 400.3 -1 3
macro read plot_sed.sm
plot 0. 2.9 400.3 -1 3
plot 0. 2.9 4.3 -1 10
macro read plot_sed.sm
plot 0.8 2.9 4.3 -1 10
plot 0.8 3.2 4.3 5 10
macro read plot_sed.sm
plot 0.8 3.2 4.3 5 10
plot 0.9 3.2 4.3 5 10
plot 0.9 3.6 4.1 6 9
macro read plot_sed.sm
plot 0.9 3.6 4.1 6 9
plot 0.8 3.6 4.1 6 9
plot 0.6 3.6 4.1 6 9
macro read plot_sed.sm
plot 0.6 3.6 4.1 6 9
!pwd
plot 0.6 3.6 4.1 6 9
sed/GAL/CFHTLS_SED/CFHTLS_MOD.list 0 → 100644
View file @ c29dd74f
CFHTLS_SED/Ell_cww.sed
CFHTLS_SED/Ell_cww_0.sed
CFHTLS_SED/Ell_cww_1.sed
CFHTLS_SED/Ell_cww_2.sed
CFHTLS_SED/Ell_cww_3.sed
CFHTLS_SED/Ell_cww_4.sed
CFHTLS_SED/Ell_cww_5.sed
CFHTLS_SED/Ell_cww_6.sed
CFHTLS_SED/Ell_cww_7.sed
CFHTLS_SED/Ell_cww_8.sed
CFHTLS_SED/Ell_cww_9.sed
CFHTLS_SED/Ell_cww_10.sed
CFHTLS_SED/Ell_cww_11.sed
CFHTLS_SED/Ell_cww_12.sed
CFHTLS_SED/Ell_cww_13.sed
CFHTLS_SED/Ell_cww_14.sed
CFHTLS_SED/Ell_cww_15.sed
CFHTLS_SED/Ell_cww_16.sed
CFHTLS_SED/Ell_cww_17.sed
CFHTLS_SED/Ell_cww_18.sed
CFHTLS_SED/Ell_cww_19.sed
CFHTLS_SED/Ell_cww_20.sed
CFHTLS_SED/Sbc_cww.sed
CFHTLS_SED/Sbc_cww_0.sed
CFHTLS_SED/Sbc_cww_1.sed
CFHTLS_SED/Sbc_cww_2.sed
CFHTLS_SED/Sbc_cww_3.sed
CFHTLS_SED/Sbc_cww_4.sed
CFHTLS_SED/Sbc_cww_5.sed
CFHTLS_SED/Sbc_cww_6.sed
CFHTLS_SED/Sbc_cww_7.sed
CFHTLS_SED/Sbc_cww_8.sed
CFHTLS_SED/Sbc_cww_9.sed
CFHTLS_SED/Sbc_cww_10.sed
CFHTLS_SED/Sbc_cww_11.sed
CFHTLS_SED/Sbc_cww_12.sed
CFHTLS_SED/Sbc_cww_13.sed
CFHTLS_SED/Sbc_cww_14.sed
CFHTLS_SED/Sbc_cww_15.sed
CFHTLS_SED/Scd_cww.sed
CFHTLS_SED/Scd_cww_0.sed
CFHTLS_SED/Scd_cww_1.sed
CFHTLS_SED/Scd_cww_2.sed
CFHTLS_SED/Scd_cww_3.sed
CFHTLS_SED/Scd_cww_4.sed
CFHTLS_SED/Scd_cww_5.sed
CFHTLS_SED/Scd_cww_6.sed
CFHTLS_SED/Scd_cww_7.sed
CFHTLS_SED/Scd_cww_8.sed
CFHTLS_SED/Scd_cww_9.sed
CFHTLS_SED/Scd_cww_10.sed
CFHTLS_SED/Im_cww_0.sed
CFHTLS_SED/Im_cww_1.sed
CFHTLS_SED/Im_cww_2.sed
CFHTLS_SED/Im_cww_3.sed
CFHTLS_SED/Im_cww_4.sed
CFHTLS_SED/Im_cww_5.sed
CFHTLS_SED/Im_cww_6.sed
CFHTLS_SED/Im_cww_7.sed
CFHTLS_SED/Im_cww_8.sed
CFHTLS_SED/Im_cww_9.sed
CFHTLS_SED/Im_cww.sed
CFHTLS_SED/SB1.sed
CFHTLS_SED/SB1_1.sed
CFHTLS_SED/SB1_2.sed
CFHTLS_SED/SB2.sed
sed/GAL/CFHTLS_SED/Ell_cww.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_0.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_1.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_10.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_11.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_12.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_13.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_14.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_15.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_16.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_17.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_18.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_19.sed 0 → 100755
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sed/GAL/CFHTLS_SED/Ell_cww_2.sed 0 → 100755
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