Commit 37a0193f authored by Yan Zhaojun's avatar Yan Zhaojun
Browse files

test

parent bca4aeef
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+2 −2
Original line number Diff line number Diff line
@@ -2151,7 +2151,7 @@ class MCIsimulator():
                t.toMag(redshift=redshift)
                # Calculating flux
                ugriz = np.array([umag, gmag, rmag, imag, zmag])
                star_flux = sed.Model_Galaxy_SED(wave, ugriz, redshift, t)  
                star_flux = sed.Model_Galaxy_SED(wave, ugriz, redshift, t, self.information['dir_path']) 
                self.log.info('load star catlog 888888888888')
                
                
@@ -2175,7 +2175,7 @@ class MCIsimulator():
                t.toMag(redshift=redshift)
                # Calculating flux
                ugriz = np.array([umag, gmag, rmag, imag, zmag])
                star_flux = sed.Model_Galaxy_SED(wave, ugriz, redshift, t)            
                star_flux = sed.Model_Galaxy_SED(wave, ugriz, redshift, t, self.information['dir_path'])           
            #########################################
            self.log.info('load star catlog 99999999')
            ##cal_SED_photons(self, flux_arr):
+2 −2
Original line number Diff line number Diff line
@@ -198,7 +198,7 @@ def Model_Stellar_SED(wave, bp, rp, temp):
    flux  = calibrate(wave, flux1, rp, band = 'GAIA_rp')
    return flux

def Model_Galaxy_SED(wave, ugriz, z, temp):
def Model_Galaxy_SED(wave, ugriz, z, temp, path):
    """Modelling galaxy SED based on u,g,r,i,z magnitude

    Args:
@@ -239,5 +239,5 @@ def Model_Galaxy_SED(wave, ugriz, z, temp):
    flux1 = reddening(temp.wave, flux0, ebv = ebv)
    
    flux2 = np.interp(wave, temp.wave * (1 + z), flux1)
    flux  = calibrate(wave, flux2, ugriz[2], band = 'SDSS_r')
    flux  = calibrate(wave, flux2, ugriz[2], path, band = 'SDSS_r')
    return flux
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