Update to v3 api

LSSTDESC · May 6, 2023 · 8232977 · 8232977
1 parent 2218f11
commit 8232977
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Showing 2 changed files with 5 additions and 5 deletions.
diff --git a/clmm/cosmology/ccl.py b/clmm/cosmology/ccl.py
@@ -106,7 +106,7 @@ def _eval_sigma_crit_core(self, z_len, z_src):
         a_len = self.get_a_from_z(z_len)
         a_src = self.get_a_from_z(z_src)
 
-        return self.be_cosmo.sigma_critical(a_len, a_src)*self.cor_factor
+        return self.be_cosmo.sigma_critical(a_lens=a_len, a_source=a_src)*self.cor_factor
 
     def _eval_linear_matter_powerspectrum(self, k_vals, redshift):
         return ccl.linear_matter_power(

diff --git a/clmm/theory/ccl_v3.py b/clmm/theory/ccl_v3.py
@@ -101,11 +101,11 @@ def _get_mass(self):
 
     def _set_concentration(self, cdelta):
         """"set concentration. Also sets/updates hdpm"""
-        self.conc = ccl.halos.ConcentrationConstant(c=cdelta, mdef=self.mdef)
+        self.conc = ccl.halos.ConcentrationConstant(c=cdelta, mass_def=self.mdef)
         with ccl.UnlockInstance(self.mdef):
             self.mdef.concentration = self.conc
         self.hdpm = self.hdpm_dict[self.halo_profile_model](
-            self.conc, **self.hdpm_opts[self.halo_profile_model])
+            concentration=self.conc, **self.hdpm_opts[self.halo_profile_model])
         self.hdpm.update_precision_fftlog(
             padding_lo_fftlog=1e-4, padding_hi_fftlog=1e3)
 
@@ -167,14 +167,14 @@ def _call_ccl_profile_lens(self, ccl_hdpm_func, radius, z_lens, ndim=2):
         a_lens = self.cosmo.get_a_from_z(z_lens)
 
         return ccl_hdpm_func(self.cosmo.be_cosmo, radius/a_lens, self.__mdelta_cor,
-                             a_lens, self.mdef)*self.cor_factor/a_lens**ndim
+                             a_lens)*self.cor_factor/a_lens**ndim
 
     def _call_ccl_profile_lens_src(self, ccl_hdpm_func, radius, z_lens, z_src):
         """"call ccl profile functions that depend on the lens and the sources"""
         a_lens = self.cosmo.get_a_from_z(z_lens)
         a_src = self.cosmo.get_a_from_z(z_src)
 
         return ccl_hdpm_func(self.cosmo.be_cosmo, radius/a_lens, self.__mdelta_cor,
-                             a_lens, a_src, self.mdef)
+                             a_lens=a_lens, a_source=a_src)
 
 Modeling = CCLCLMModeling