Пример #1
0
                                                cHbeta=cHbeta.nominal_value,
                                                R_v=R_v)
        IntEmi_dered = dz.derreddening_spectrum(Wave_E,
                                                Int_E,
                                                reddening_curve=red_curve,
                                                cHbeta=cHbeta.nominal_value,
                                                R_v=R_v)

        Int_Sum = IntEmi_dered + Int_Stellar_Resampled + Int_N

        dz.data_plot(Wave_O, IntObs_dered, 'Observed spectrum')
        dz.data_plot(Wave_N, Int_N, 'Nebular continuum', linestyle=':')
        dz.data_plot(Wave_S, Int_S, 'Stellar continuum', linestyle='--')
        dz.insert_image(
            '/home/vital/Dropbox/Astrophysics/Papers/Yp_AlternativeMethods/images/SHOC579_invert.png',
            Image_Coordinates=[0.07, 0.875],
            Zoom=0.25,
            Image_xyCoords='axes fraction')

        #Set titles and legend
        PlotTitle = ''
        dz.FigWording(r'Wavelength $(\AA)$',
                      'Flux' + r'$(erg\,cm^{-2} s^{-1} \AA^{-1})$',
                      PlotTitle,
                      loc='upper right')

        dz.Axis.set_xlim(3550, 10000)

        axins2 = inset_axes(dz.Axis, width='70%', height='50%', loc=7)

        #sub_axes = plt.axes([6000.0, 1.2e-14, 3000, 3.75e-14])
Пример #2
0
            axins2.set_ylim(-0.2e-16, 3.0e-16)
            mark_inset(dz.ax1, axins2, loc1=2, loc2=4, fc="none", ec="0.5") 
                 
            axins.get_xaxis().set_visible(False)
            axins.get_yaxis().set_visible(False)
            axins2.get_xaxis().set_visible(False)
            axins2.get_yaxis().set_visible(False)
                 
            dz.FigWording('', 'Flux ' + r'$(erg\,cm^{-2} s^{-1} \AA^{-1})$', '', loc='upper left', graph_axis=dz.ax1, sort_legend=True) 
            dz.FigWording(r'Wavelength $(\AA)$', 'Normalized flux', '', loc='lower center', graph_axis=dz.ax2, ncols_leg=4) 
            
            dz.ax2.set_ylim(0.2,1.25)
            if 'S3_9531A_continuum' in obj_dict:
                dz.ax1.set_ylim(-2 * obj_dict['S3_9531A_continuum'], 1.1 * obj_dict['S3_9531A_Peak'])
            else:
                dz.ax1.set_ylim(0.005 * mean_flux, 20 * mean_flux)
            
            dz.insert_image('/home/vital/Downloads/obj08_SDSS_image_color.png', Image_Coordinates = [0.50,0.80], Zoom=0.25, Image_xyCoords = 'axes fraction', axis_plot=dz.ax1)
            
            dz.savefig(image_address, extension='.png')
            #dz.display_fig()
            
#         output_pickle = '{objFolder}{stepCode}_{objCode}_{ext}'.format(objFolder=ouput_folder, stepCode=script_code, objCode=objName, ext='Telluric correction')
#         dz.save_manager(output_pickle, save_pickle = True)
#         dz.savefig('/home/vital/Dropbox/Astrophysics/Seminars/Angeles_Seminar/' + '8_telluric_correction', extension='.png')





Пример #3
0
    objName = catalogue_df.iloc[i].name
    
    if objName == '8':
    
        #Joining pointing
        joining_wavelength = catalogue_df.iloc[i].join_wavelength
     
        #Treat each arm file    
        blue_fits_file = catalogue_df.iloc[i]['zBlue_file'] 
        red_fits_file = catalogue_df.iloc[i]['zRed_file'] 
     
        CodeName_Blue, FileName_Blue, FileFolder_Blue = dz.Analyze_Address(blue_fits_file)
        CodeName_Red, FileName_Red, FileFolder_Red = dz.Analyze_Address(red_fits_file)
     
        wave_Blue, flux_Blue, ExtraData_Blue = dz.get_spectra_data(blue_fits_file)
        wave_Red, flux_Red, ExtraData_Red = dz.get_spectra_data(red_fits_file)
     
        idx_blue = searchsorted(wave_Blue, joining_wavelength) 
        idx_red  = searchsorted(wave_Red, joining_wavelength) 
         
        wave_comb = concatenate([wave_Blue[0:idx_blue], wave_Red[idx_red:-1]])
        flux_comb = concatenate([flux_Blue[0:idx_blue], flux_Red[idx_red:-1]])
     
        dz.data_plot(wave_Blue, flux_Blue, label = 'WHT blue arm')
        dz.data_plot(wave_Red, flux_Red, label = 'WHT red arm')
        dz.insert_image('/home/vital/Dropbox/Astrophysics/Seminars/Angeles_Seminar/8.png', Image_Coordinates = [0.85,0.70], Zoom=0.20, Image_xyCoords = 'axes fraction')
        dz.FigWording(r'Wavelength $(\AA)$', 'Flux ' + r'$(erg\,cm^{-2} s^{-1} \AA^{-1})$', 'HII galaxy: SDSSJ024815.93-081716.5, WHT observation')
        dz.display_fig()
        #dz.savefig('/home/vital/Dropbox/Astrophysics/Seminars/Angeles_Seminar/' + '8_WHT', extension='.png')