cut AGN module to lam>5nm

pcigale/sed_modules/fritz2006.py

@@ -124,6 +124,15 @@ class Fritz2006(SedModule):
         self.l_agn_agn = np.trapz(self.fritz2006.lumin_agn,
                                   x=self.fritz2006.wave)
 
+        # Apply wavelength cut
+        lam_cut = 5.
+        lam_use_idxs = self.fritz2006.wave>=lam_cut
+        self.fritz2006.wave = self.fritz2006.wave[lam_use_idxs]
+        self.fritz2006.lumin_agn = self.fritz2006.lumin_agn[lam_use_idxs]
+        self.fritz2006.lumin_scatt = self.fritz2006.lumin_scatt[lam_use_idxs]
+        self.fritz2006.lumin_therm  = self.fritz2006.lumin_therm[lam_use_idxs]
+        self.fritz2006.lumin_intrin_agn = self.fritz2006.lumin_intrin_agn[lam_use_idxs]
+
         # Apply polar-dust obscuration
         # We define various constants necessary to compute the model
         self.c = cst.c * 1e9

pcigale/sed_modules/skirtor2016.py

@@ -54,7 +54,7 @@ class SKIRTOR2016(SedModule):
         ('oa', (
             'cigale_list(options=10 & 20 & 30 & 40 & 50 & 60 & 70 & 80)',
             "Angle measured between the equatorial plan and edge of the torus. "
-            "Half-opening angle of the dust-free cone is 90-oa"
+            "Half-opening angle of the dust-free cone is 90-oa. "
             "Possible values are: 10, 20, 30, 40, 50, 60, 70, and 80",
             40
         )),
@@ -120,10 +120,18 @@ class SKIRTOR2016(SedModule):
                                                     self.oa, self.R, self.Mcl,
                                                     self.i)
 
+        # Apply wavelength cut
+        lam_cut = 5.
+        lam_use_idxs = self.SKIRTOR2016.wave>=lam_cut
+        self.SKIRTOR2016.wave = self.SKIRTOR2016.wave[lam_use_idxs]
+        self.SKIRTOR2016.disk = self.SKIRTOR2016.disk[lam_use_idxs]
+        self.SKIRTOR2016.dust = self.SKIRTOR2016.dust[lam_use_idxs]
+        self.SKIRTOR2016.intrin_iso_disk = self.SKIRTOR2016.intrin_iso_disk[lam_use_idxs]
+
         # Modify the model so that the central source is isotropic
         # Calculate the coverting factors disk emission
         # (only for type-1 case, since disk emission in type-2 is zero)
-        # (since dust emission is normalized to unity; it remains same)
+        # (dust emission is normalized to unity, so it remains same)
         if self.i<=(90-self.oa):
             self.SKIRTOR2016.disk*= (4*np.sin(self.oa*np.pi/180)**2 + 3*np.sin(self.oa*np.pi/180)) / \
                                     (12*np.cos(self.i*np.pi/180)**2 + 6*np.cos(self.i *np.pi/180))