cut AGN disk SED to lam>10^1.5 nm; extend X-ray down to lam=10^1.2

database_builder/__init__.py

@@ -794,7 +794,7 @@ def build_skirtor2016(base):
         disk += scatt
 
         # Apply wavelength cut to avoid X-ray wavelength
-        lam_cut = 5.
+        lam_cut = 10**1.5
         lam_idxs = wl_uncut>=lam_cut
         # Calculate the re-normalization factor to keep energy conservation
         norm_fac = np.trapz(intrin_disk, x=wl_uncut) / \

pcigale/sed_modules/xray.py

@@ -65,8 +65,8 @@ class Xray(SedModule):
         self.nu_2keV = c / lam_2keV
 
         # We define the wavelength range for the non thermal emission
-        # corresponding to 0.4-1200 keV
-        self.wave = np.logspace(-3, 0.5, 1000)
+        # corresponding to 0.08-1200 keV
+        self.wave = np.logspace(-3, 1.2, 1000)
 
         # X-ray emission from galaxies: 1.hot-gas & 2.X-ray binaries
         # 1.Hot-gas, assuming power-law index gamma=3
@@ -91,8 +91,8 @@ class Xray(SedModule):
         # Calculate total AGN corona X-ray luminosity
         self.l_agn_xray_total = np.trapz(self.lumin_corona, x=self.wave)
         # Calculate 2-10 keV AGN corona X-ray luminosity
-        # 2-10 keV corredponds to self.wave[598:798]
-        self.l_agn_xray_2to10keV = np.trapz(self.lumin_corona[598:798], x=self.wave[598:798])
+        lam_idxs = (self.wave<=self.lam_2keV) & (self.wave>=self.lam_10keV)
+        self.l_agn_xray_2to10keV = np.trapz(self.lumin_corona[lam_idxs], x=self.wave[lam_idxs])
 
 
     def process(self, sed):