File tree Expand file tree Collapse file tree 1 file changed +5
-2
lines changed Expand file tree Collapse file tree 1 file changed +5
-2
lines changed Original file line number Diff line number Diff line change @@ -304,7 +304,8 @@ def _setup_inv_abel_dens_onion_temp(sources: Union[GalaxyCluster, ClusterSample]
304
304
freeze_met = freeze_met , abund_table = abund_table , temp_lo_en = temp_lo_en ,
305
305
temp_hi_en = temp_hi_en , num_cores = num_cores , stacked_spectra = stacked_spectra ,
306
306
telescope = src_telescopes )
307
-
307
+ print ("temp_profs" )
308
+ print (temp_profs )
308
309
# We are reorganising this temp_profs output so it is easier to cycle through in later functions
309
310
# temp_prof_dict will have sources as keys, then a dictionary value, this dictionary has
310
311
# telescope keys with values that are the profile object, ie. {src1: {'xmm' : Profile}}
@@ -316,7 +317,9 @@ def _setup_inv_abel_dens_onion_temp(sources: Union[GalaxyCluster, ClusterSample]
316
317
# temp_profs is of the form {'xmm': [Profile, Profile, etc.]}
317
318
src_dict [tel ] = temp_profs [tel ][p_ind ]
318
319
temp_prof_dict [str (cut_sources [p_ind ])] = src_dict
319
-
320
+
321
+ print ('temp_prof_dict' )
322
+ print (temp_prof_dict )
320
323
# Now we take only the sources that have successful 3D temperature profiles.
321
324
# We do the temperature profile stuff first because its more difficult, and why should we waste
322
325
# time on a density profile if the temperature profile cannot even be measured.
You can’t perform that action at this time.
0 commit comments