| src/galsbi/__init__.py |
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| src/galsbi/citations.py |
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0 |
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load_halo_histogram |
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read_pinocchio_config_details |
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generate_galaxy_histogram |
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| src/galsbi/sham_ot/utils.py |
determine_skyarea_of_pinocchio_sim |
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| src/galsbi/sham_ot/utils.py |
opening_to_skyarea |
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| src/galsbi/sham_ot/utils.py |
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| src/galsbi/ucat/__init__.py |
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0 |
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189 |
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| src/galsbi/ucat/config/galaxy_catalog.py |
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| src/galsbi/ucat/filters_util.py |
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| src/galsbi/ucat/filters_util.py |
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| src/galsbi/ucat/filters_util.py |
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| src/galsbi/ucat/filters_util.py |
create_filter_collection.add_sdss_filters |
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| src/galsbi/ucat/filters_util.py |
create_filter_collection.add_vista_filters |
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| src/galsbi/ucat/filters_util.py |
create_filter_collection.add_omegacam_filters |
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| src/galsbi/ucat/filters_util.py |
create_filter_collection.add_lsstcam_filters |
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| src/galsbi/ucat/filters_util.py |
create_filter_collection.add_euclid_filters |
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| src/galsbi/ucat/filters_util.py |
store_filter_collection |
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7 |
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load_filters |
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10 |
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| src/galsbi/ucat/filters_util.py |
UseShortFilterNames.__init__ |
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| src/galsbi/ucat/filters_util.py |
UseShortFilterNames.__call__ |
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| src/galsbi/ucat/filters_util.py |
UseShortFilterNames.__getattr__ |
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| src/galsbi/ucat/filters_util.py |
get_default_full_filter_names |
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| src/galsbi/ucat/filters_util.py |
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15 |
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| src/galsbi/ucat/galaxy_population_models/__init__.py |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_light_profile.py |
sample_sersic_berge |
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| src/galsbi/ucat/galaxy_population_models/galaxy_light_profile.py |
sample_sersic_betaprime |
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| src/galsbi/ucat/galaxy_population_models/galaxy_light_profile.py |
sample_sersic_for_galaxy_type |
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| src/galsbi/ucat/galaxy_population_models/galaxy_light_profile.py |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
find_closest_ind |
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4 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
initialize_luminosity_functions |
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maximum_redshift |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
phi_star_lum_fct |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
upper_inc_gamma |
|
6 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
NumGalCalculator.__init__ |
|
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
NumGalCalculator.__call__ |
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8 |
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NumGalCalculator._redshift_density |
|
10 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
RedshiftAbsMagSampler.__init__ |
|
14 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
RedshiftAbsMagSampler.__call__ |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
RedshiftAbsMagSampler._setup_redshift_grid |
|
12 |
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0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
RedshiftAbsMagSampler._setup_mag_grid |
|
7 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
LuminosityFunction.__init__ |
|
23 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
LuminosityFunction.sample_z_mabs_and_apply_cut |
|
23 |
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0 |
|
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
LuminosityFunction.analytical_number_density |
|
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_luminosity_function.py |
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26 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
_hash_array |
|
6 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
_safe_key_val |
|
8 |
2 |
0 |
|
75% |
| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
_build_ot_cache_key |
|
1 |
0 |
0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
sample_position_uniform |
|
21 |
1 |
0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
sample_with_sham_ot |
|
115 |
0 |
0 |
|
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
get_ot_epsilon |
|
5 |
0 |
0 |
|
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
sample_rest_of_lf |
|
16 |
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0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
get_halo_catalog |
|
7 |
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0 |
|
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| src/galsbi/ucat/galaxy_population_models/galaxy_position.py |
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21 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
dirichlet_alpha_ev |
|
3 |
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|
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| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
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|
6 |
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0 |
|
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| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
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|
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0 |
|
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| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
sample_template_coeff_dirichlet__alpha_mode.dir_mode_to_alpha |
|
5 |
0 |
0 |
|
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| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
sample_template_coeff_dirichlet__alpha_mode.dir_mode |
|
1 |
1 |
0 |
|
0% |
| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
sample_template_coeff_dirichlet__alpha_mode.get_max_sigma |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
sample_template_coeff_dirichlet |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
sample_template_coeff_lumfuncs |
|
12 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_sed.py |
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|
7 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
distortion_to_shear |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
sample_ellipticities_gaussian |
|
8 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
pe_disc |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
pe_bulge |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
sample_ellipticities_beta |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
sample_ellipticities_beta_mode |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
sample_ellipticities_for_galaxy_type |
|
19 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
backwards_compatibility |
|
15 |
0 |
0 |
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100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_shape.py |
(no function) |
|
12 |
0 |
0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_size.py |
apply_pycosmo_distfun |
|
3 |
0 |
0 |
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| src/galsbi/ucat/galaxy_population_models/galaxy_size.py |
r50_phys_to_ang |
|
4 |
0 |
0 |
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100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_size.py |
sample_r50_for_galaxy_type |
|
29 |
1 |
0 |
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97% |
| src/galsbi/ucat/galaxy_population_models/galaxy_size.py |
sample_r50_phys |
|
5 |
0 |
0 |
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100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_size.py |
backwards_compatibility |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_population_models/galaxy_size.py |
(no function) |
|
7 |
0 |
0 |
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100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
apply_pycosmo_distfun |
|
3 |
0 |
0 |
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100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
intp_z_m_cut |
|
30 |
0 |
0 |
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100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
intp_z_m_cut.find_max_template_ind |
|
5 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
intp_z_m_cut.app_mag_ref |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
intp_z_m_cut.magnitude_difference |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.__init__ |
|
21 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.sample |
|
26 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.compute_factors |
|
16 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.mvnrnd |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.trandn |
|
20 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.tn |
|
15 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.trnd |
|
13 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.ntail |
|
16 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.psy |
|
7 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.get_gradient_function |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.get_gradient_function.gradpsi |
|
25 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
TruncatedMVN.colperm |
|
35 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
lnNormalProb |
|
17 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
lnPhi |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat/galaxy_sampling_util.py |
(no function) |
|
29 |
0 |
0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
sigma_to_fwhm |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
fwhm_to_sigma |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
apply_reduced_shear_to_ellipticities |
|
9 |
3 |
0 |
|
67% |
| src/galsbi/ucat/lensing_util.py |
apply_shear_to_ellipticities |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
shear_to_reduced_shear |
|
2 |
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0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
distortion_to_shear |
|
4 |
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0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
shear_to_distortion |
|
4 |
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0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
distortion_to_moments |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat/lensing_util.py |
moments_to_distortion |
|
11 |
0 |
0 |
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100% |
| src/galsbi/ucat/lensing_util.py |
moments_to_shear |
|
11 |
0 |
0 |
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100% |
| src/galsbi/ucat/lensing_util.py |
shear_to_moments |
|
12 |
0 |
0 |
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| src/galsbi/ucat/lensing_util.py |
calculate_flux_magnification |
|
2 |
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0 |
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| src/galsbi/ucat/lensing_util.py |
calculate_size_magnification |
|
2 |
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0 |
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| src/galsbi/ucat/lensing_util.py |
(no function) |
|
14 |
0 |
0 |
|
100% |
| src/galsbi/ucat/magnitude_calculator.py |
flux_to_AB_mag |
|
3 |
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0 |
|
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| src/galsbi/ucat/magnitude_calculator.py |
AB_mag_to_flux |
|
1 |
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0 |
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100% |
| src/galsbi/ucat/magnitude_calculator.py |
MagCalculatorDirect.__init__ |
|
4 |
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0 |
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| src/galsbi/ucat/magnitude_calculator.py |
MagCalculatorDirect.__call__ |
|
19 |
1 |
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95% |
| src/galsbi/ucat/magnitude_calculator.py |
MagCalculatorTable.__init__ |
|
4 |
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0 |
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| src/galsbi/ucat/magnitude_calculator.py |
MagCalculatorTable.__call__ |
|
18 |
1 |
0 |
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94% |
| src/galsbi/ucat/magnitude_calculator.py |
(no function) |
|
17 |
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0 |
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| src/galsbi/ucat/plugins/__init__.py |
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|
0 |
0 |
0 |
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| src/galsbi/ucat/plugins/apply_shear.py |
evaluate_healpix_shear_map |
|
6 |
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0 |
|
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| src/galsbi/ucat/plugins/apply_shear.py |
linear_interpolation |
|
2 |
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0 |
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interpolate_maps_fast |
|
13 |
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0 |
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interpolate_maps |
|
12 |
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0 |
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evaluate_hdf5_shear_maps |
|
18 |
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0 |
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| src/galsbi/ucat/plugins/apply_shear.py |
Plugin.__call__ |
|
22 |
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0 |
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Plugin.__str__ |
|
1 |
1 |
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(no function) |
|
16 |
0 |
0 |
|
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| src/galsbi/ucat/plugins/galaxy_mag_noise.py |
mag_to_flux |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/galaxy_mag_noise.py |
flux_to_mag |
|
1 |
0 |
0 |
|
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| src/galsbi/ucat/plugins/galaxy_mag_noise.py |
Plugin.__call__ |
|
8 |
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0 |
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| src/galsbi/ucat/plugins/galaxy_mag_noise.py |
Plugin.__str__ |
|
1 |
1 |
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| src/galsbi/ucat/plugins/galaxy_mag_noise.py |
(no function) |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/galaxy_z_noise.py |
add_z_noise |
|
6 |
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0 |
|
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| src/galsbi/ucat/plugins/galaxy_z_noise.py |
Plugin.__call__ |
|
4 |
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0 |
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| src/galsbi/ucat/plugins/galaxy_z_noise.py |
Plugin.__str__ |
|
1 |
1 |
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|
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| src/galsbi/ucat/plugins/galaxy_z_noise.py |
(no function) |
|
9 |
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0 |
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| src/galsbi/ucat/plugins/sample_galaxies.py |
Plugin.__call__ |
|
4 |
0 |
0 |
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100% |
| src/galsbi/ucat/plugins/sample_galaxies.py |
Plugin.__str__ |
|
1 |
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0 |
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| src/galsbi/ucat/plugins/sample_galaxies.py |
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|
4 |
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0 |
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| src/galsbi/ucat/plugins/sample_galaxies_morph.py |
Plugin.__call__ |
|
27 |
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0 |
|
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| src/galsbi/ucat/plugins/sample_galaxies_morph.py |
Plugin.__str__ |
|
1 |
1 |
0 |
|
0% |
| src/galsbi/ucat/plugins/sample_galaxies_morph.py |
(no function) |
|
12 |
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0 |
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| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
ExtinctionMapEvaluator.__init__ |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
ExtinctionMapEvaluator.__call__ |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
get_magnitude_calculator_direct |
|
7 |
0 |
0 |
|
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| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
get_magnitude_calculator_table |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
Plugin.check_n_gal_prior |
|
7 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
Plugin.check_max_mem_error |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
Plugin.__call__ |
|
116 |
3 |
0 |
|
97% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
Plugin.__str__ |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
compute_templates_extinction_appmag_for_galaxies |
|
10 |
1 |
0 |
|
90% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
in_pos |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
get_seds |
|
9 |
0 |
0 |
|
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| src/galsbi/ucat/plugins/sample_galaxies_photo.py |
(no function) |
|
31 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/write_catalog.py |
catalog_to_rec |
|
16 |
0 |
0 |
|
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sed_catalog_to_rec |
|
17 |
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0 |
|
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save_sed |
|
3 |
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0 |
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Plugin.__call__ |
|
19 |
0 |
0 |
|
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Plugin.enrich_catalog |
|
22 |
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0 |
|
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| src/galsbi/ucat/plugins/write_catalog.py |
Plugin.__str__ |
|
1 |
0 |
0 |
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100% |
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(no function) |
|
13 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/write_catalog_photo.py |
get_ucat_catalog_filename |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/write_catalog_photo.py |
Plugin.__call__ |
|
13 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/write_catalog_photo.py |
Plugin.__str__ |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/plugins/write_catalog_photo.py |
(no function) |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat/sed_templates_util.py |
get_redshift_extinction_grid |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat/sed_templates_util.py |
get_template_integrals |
|
16 |
0 |
2 |
|
100% |
| src/galsbi/ucat/sed_templates_util.py |
store_sed_integrals |
|
12 |
0 |
0 |
|
100% |
| src/galsbi/ucat/sed_templates_util.py |
load_sed_integrals |
|
30 |
2 |
0 |
|
93% |
| src/galsbi/ucat/sed_templates_util.py |
load_sed_integrals.filter_name_back_compatibility |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat/sed_templates_util.py |
load_template_spectra |
|
11 |
0 |
0 |
|
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| src/galsbi/ucat/sed_templates_util.py |
(no function) |
|
12 |
0 |
0 |
|
100% |
| src/galsbi/ucat/spectrum_util.py |
spline_ext_coeff |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat/spectrum_util.py |
extinction_coefficient |
|
9 |
0 |
0 |
|
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| src/galsbi/ucat/spectrum_util.py |
extinction_coefficient.uv_extinction |
|
11 |
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0 |
|
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| src/galsbi/ucat/spectrum_util.py |
extinction_coefficient.uv_extinction.uv_curvature |
|
5 |
0 |
0 |
|
100% |
| src/galsbi/ucat/spectrum_util.py |
construct_intrinsic_spectrum |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat/spectrum_util.py |
apply_extinction |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/spectrum_util.py |
construct_reddened_spectrum |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat/spectrum_util.py |
(no function) |
|
7 |
0 |
0 |
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100% |
| src/galsbi/ucat/utils.py |
memory_usage_psutil |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat/utils.py |
(no function) |
|
3 |
0 |
0 |
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100% |
| src/galsbi/ucat_sps/__init__.py |
(no function) |
|
0 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/config/__init__.py |
(no function) |
|
0 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/config/common_sps.py |
(no function) |
|
355 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/config/galaxy_catalog_sps.py |
(no function) |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/__init__.py |
(no function) |
|
0 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_agn.py |
sample_ratio_agn_to_galaxy_bolometric_luminosity |
|
45 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_agn.py |
(no function) |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_attenuation.py |
stellar_mass_and_ssfr_for_dust_attenuation |
|
8 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_attenuation.py |
sample_dust_attenuation_parameters_charlotfall2000 |
|
19 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_attenuation.py |
_sample_truncated_normal |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_attenuation.py |
_two_population_diffuse_dust_predictors |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_attenuation.py |
sample_dust_attenuation_parameters_charlotfall2000_two_population |
|
18 |
1 |
0 |
|
94% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_attenuation.py |
sample_dust_attenuation_parameters |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_attenuation.py |
(no function) |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_emission.py |
sample_Dale2014_dust_emission_parameters |
|
7 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_dust_emission.py |
(no function) |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_gas_ionization.py |
sample_gas_ionization_Kashino19 |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_gas_ionization.py |
(no function) |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_light_profile.py |
sample_sersic_stellar_mass |
|
5 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_light_profile.py |
sample_sersic_for_galaxy_type |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_light_profile.py |
(no function) |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_metallicity_history.py |
vectorized_truncnorm_sample |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_metallicity_history.py |
sample_gas_metallicity |
|
26 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_metallicity_history.py |
integrate_sfh |
|
13 |
2 |
0 |
|
85% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_metallicity_history.py |
generate_gas_metallicity_history_snorm_trunc |
|
22 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_metallicity_history.py |
generate_gas_metallicity_history_on_ssp_grid |
|
37 |
2 |
0 |
|
95% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_metallicity_history.py |
(no function) |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
sample_r50_from_stellar_mass |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
sample_r50_phys_from_stellar_mass |
|
20 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
mean_r50_phys_tortorelli25 |
|
14 |
1 |
0 |
|
93% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
mean_r50_phys_lange15 |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
_mean_log10_r50_phys_nedkova21_relations |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
_interpolate_relations_in_redshift |
|
12 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
mean_r50_phys_nedkova21_binned |
|
8 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
scatter_r50_phys_nedkova21 |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
_mean_r50_phys_miller2026_relation |
|
12 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
mean_r50_phys_miller2026 |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
scatter_r50_phys_miller2026 |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_size.py |
(no function) |
|
13 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
_load_ssp_time_grid_cached |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
load_ssp_time_grid |
|
19 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
stable_sigmoid |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
stable_logit |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
beta_shape_from_mean_concentration |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
sample_truncated_student_t |
|
31 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
_one_dimensional_array |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
_draw_conditional_sfh_shapes |
|
19 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
sample_conditional_sfh_parameters |
|
38 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
massfunc_snorm_trunc |
|
16 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
massfunc_snorm_burst_trunc |
|
17 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
_evaluate_unit_sfh_on_ssp_grid |
|
15 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
evaluate_sfh_on_ssp_grid |
|
60 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
single_galaxy_sfh_snorm_trunc |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
evaluate_sfh_on_uniform_grid |
|
34 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
get_mean_sfh_shape_params |
|
15 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
sample_sfh_shape_params |
|
34 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
sample_sfh_snorm_trunc |
|
7 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_star_formation_history.py |
(no function) |
|
28 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
find_closest_ind |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
single_stellar_mass_function_parametrisation |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
double_stellar_mass_function_parametrisation |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
stellar_mass_function_m_star |
|
8 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
stellar_mass_function_phi_star |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
upper_inc_gamma |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
initialize_stellar_mass_functions |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
maximum_redshift |
|
11 |
2 |
0 |
|
82% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
maximum_redshift.conditional_mass_fraction |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
NumGalCalculator.__init__ |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
NumGalCalculator.__call__ |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
NumGalCalculator._redshift_density |
|
7 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
RedshiftSMSampler.__init__ |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
RedshiftSMSampler.__call__ |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
RedshiftSMSampler._setup_redshift_grid |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
RedshiftSMSampler._setup_mag_grid |
|
7 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
StellarMassFunction.__init__ |
|
19 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
StellarMassFunction.sample_z_sm_and_apply_cut |
|
23 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_stellar_mass_function.py |
(no function) |
|
27 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_surviving_stellar_mass.py |
_read_json |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_surviving_stellar_mass.py |
_emulator_file |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_surviving_stellar_mass.py |
load_surviving_stellar_mass_model |
|
35 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_surviving_stellar_mass.py |
predict_log10_surviving_to_formed_mass_ratio |
|
25 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_surviving_stellar_mass.py |
predict_log10_surviving_stellar_mass |
|
16 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_surviving_stellar_mass.py |
compute_legacy_surviving_stellar_mass |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_surviving_stellar_mass.py |
(no function) |
|
13 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_velocity_dispersion.py |
sample_velocity_dispersion_zahid |
|
16 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/galaxy_population_models/galaxy_velocity_dispersion.py |
(no function) |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/plugins/__init__.py |
(no function) |
|
0 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/plugins/add_promage_magnitude_error.py |
Plugin.__call__ |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/plugins/add_promage_magnitude_error.py |
Plugin.__str__ |
|
1 |
1 |
0 |
|
0% |
| src/galsbi/ucat_sps/plugins/add_promage_magnitude_error.py |
(no function) |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/plugins/sample_galaxies_sps.py |
check_max_mem_error |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/plugins/sample_galaxies_sps.py |
Plugin.__call__ |
|
180 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/plugins/sample_galaxies_sps.py |
Plugin.__str__ |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/plugins/sample_galaxies_sps.py |
(no function) |
|
31 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/spectrum_util_sps.py |
apply_extinction |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/spectrum_util_sps.py |
apply_velocity_broadening |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/spectrum_util_sps.py |
apply_velocity_broadening.process_spectrum |
|
16 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/spectrum_util_sps.py |
apply_velocity_broadening.process_all_galaxies |
|
5 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/spectrum_util_sps.py |
compute_Temple21_AGN_contributions |
|
17 |
3 |
0 |
|
82% |
| src/galsbi/ucat_sps/spectrum_util_sps.py |
(no function) |
|
10 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/sps_sed_generator.py |
MagnitudeGenerator.__init__ |
|
5 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/sps_sed_generator.py |
MagnitudeGenerator.__call__ |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/sps_sed_generator.py |
get_magnitudes_with_ProSpect |
|
65 |
4 |
0 |
|
94% |
| src/galsbi/ucat_sps/sps_sed_generator.py |
get_magnitudes_with_emulator |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/sps_sed_generator.py |
(no function) |
|
17 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
galaxy_property_seed |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
stellar_mass_function_seed |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
get_age_of_the_universe_from_redshift |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
get_lookbacktime_from_redshift |
|
2 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
_normalise_filter_names |
|
3 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
_local_filter_names |
|
11 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
_h5_filter_name |
|
8 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
_filter_effective_wavelengths |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
apply_extinction_to_magnitudes |
|
6 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
reorder_prospect_magnitudes_to_filters |
|
4 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
validate_recent_burst_properties |
|
9 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
build_promage_physical_properties |
|
1 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
load_promage_models |
|
27 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
predict_promage_magnitudes |
|
18 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
apply_galaxy_observed_magnitude_cut |
|
13 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
compute_ab_magnitudes |
|
13 |
0 |
0 |
|
100% |
| src/galsbi/ucat_sps/util_sps.py |
(no function) |
|
26 |
0 |
0 |
|
100% |