])
return DataTable
DataLog_Extension = '_dr10_LinesLog_v3.txt' #First batch process for untreated spectra
TexTable_Extension = '_TableSingleIntensities.tex' #First data log for untreated spectra
# DataLog_Extension = '_WHT_LinesLog_v3.txt' #First batch process for untreated spectra
# TexTable_Extension = '_WHT_TableSingleIntensities.tex' #First data log for untreated spectra
CatalogueFolder, DataType, Log_Format = DataToTreat()
Pattern = DataType + '.fits'
# Importing Dazer libraries for launching the batch measurement
pv = plotMan.myPickle()
#Find and organize files from terminal command or .py file
FilesList = pv.FindAndOrganize(Pattern, CatalogueFolder, CheckComputer=True)
HBeta_Ion = "Hbeta_4_2"
HeaderSize = 2
for m in range(len(FilesList)):
for j in range(len(FilesList[m])):
# Get the spectrum:
CodeName, FileName, FileFolder = pv.FileAnalyzer(FilesList[m][j])
LineIntensity_Table = GetDataTable(FileFolder, CodeName,
import CodeTools.PlottingManager as plotMan
import numpy as np
def mAB_to_ergs(Flux_Ab):
Exponent = -0.4 * (Flux_Ab + 48.6)
Flux_Erg = np.power(10, Exponent)
return Flux_Erg
# Data search configuration
Pv = plotMan.myPickle()
# Generate figures
Pv.FigFormat_One(ColorConf="Day1")
c_AperS = 2.99792458e18 # A / s
Night1_Folder = "/home/vital/Astrodata/WHT_HII_Galaxies/HII_WHT_2012_12/Noche1/Blue/"
Night2_Folder = "/home/vital/Astrodata/WHT_HII_Galaxies/HII_WHT_2012_12/Noche2/Blue/"
# --------------------------------NIGHT 1-----------------------------------------
# StarFile_1 = 'a_std_wolf.dat'
# StarSpectra = 'Star_Wolf_wide_cr_f_a_bg0001_fxW_v1.fits'
# Title = 'Wolf 1346 flux calibration comparison with reference Night 1'
# Folder = Night1_Folder
#
# WaveTheo, FluxTheo_AB = np.loadtxt(Folder + StarFile_1, comments='#', usecols = (0, 1), unpack=True)
#!/usr/bin/python
import CodeTools.MethodsPyplot as mp
import matplotlib.pyplot as plt
from PipeLineMethods.ManageFlow import DataToTreat
import CodeTools.PlottingManager as plotMan
import PipeLineMethods.pyFlow_Configuration as pyFlowMan
import AstroTools.AstroClass as astrotools
import AstroTools.ScienceClass as mathtools
# Data search configuration
PipeManager = pyFlowMan.FlowManager()
PlotVector = plotMan.myPickle()
Astro = astrotools.AstroPythonMethods()
vit = mathtools.FittingMethods()
def Galaxy_Properties():
#This method contains the redshift calculated from the emission lines and the EBV from the dust maps.
#It must be recalculated
GalaxyList=["obj52703-612v1_z0.009_EBV0.0097",
"obj52703-612v2_z0.009_EBV0.0097",
"obj51991-224_z0.102_EBV0.0176 ",
"obj51959-092_z0.042_EBV0.0267 ",
"obj52235-602_z0.024_EBV0.0266",
"obj52319-521_z0.033_EBV0.0247",
"objSHOC575_z0.016_EBV0.0331",
"objSHOC593_z0.028058_EBV0.1013",
"objSHOC036_z0.037519_EBV0.0235",