magnitude ('mag_use_normal') calculations for galaxies and QSOs now is only based on their SEDs

catalog/C9_Catalog.py

@@ -557,8 +557,22 @@ class Catalog(CatalogBase):
         # erg/s/cm2/A --> photon/s/m2/A
         all_sed = y * lamb / (cons.h.value * cons.c.value) * 1e-13
         sed = Table(np.array([lamb, all_sed]).T, names=('WAVELENGTH', 'FLUX'))
-        if obj.type == 'quasar':
-            # integrate to get the magnitudes
+        # if obj.type == 'quasar':
+        #     # integrate to get the magnitudes
+        #     sed_photon = np.array([sed['WAVELENGTH'], sed['FLUX']]).T
+        #     sed_photon = galsim.LookupTable(x=np.array(sed_photon[:, 0]), f=np.array(
+        #         sed_photon[:, 1]), interpolant='nearest')
+        #     sed_photon = galsim.SED(
+        #         sed_photon, wave_type='A', flux_type='1', fast=False)
+        #     interFlux = integrate_sed_bandpass(
+        #         sed=sed_photon, bandpass=self.filt.bandpass_full)
+        #     obj.param['mag_use_normal'] = getABMAG(
+        #         interFlux, self.filt.bandpass_full)
+        #     # mag = getABMAG(interFlux, self.filt.bandpass_full)
+        #     # print("mag diff = %.3f"%(mag - obj.param['mag_use_normal']))
+
+        # integrate to get the magnitudes
+        if obj.type == 'quasar' or obj.type == 'galaxy':
             sed_photon = np.array([sed['WAVELENGTH'], sed['FLUX']]).T
             sed_photon = galsim.LookupTable(x=np.array(sed_photon[:, 0]), f=np.array(
                 sed_photon[:, 1]), interpolant='nearest')