cosmology-kit · nikosarcevic · May 14, 2026 · May 12, 2026 · May 12, 2026 · May 12, 2026
diff --git a/docs/about/lf_overview.rst b/docs/about/lf_overview.rst
@@ -303,7 +303,7 @@ and normalize the result over the supplied redshift grid.
    )
 
 This is useful for constructing LF-dependent redshift trends.
-Without a volume weight, the result is the luminosity-function
+Without a volume weight, the result is the luminosity function
 selection factor only, not a full survey redshift distribution.
 
 A volume-weighted trend can be computed by passing a callable:

diff --git a/docs/api/lfkit.photometry.conditional_lf_integrals.rst b/docs/api/lfkit.photometry.conditional_lf_integrals.rst
@@ -0,0 +1,7 @@
+lfkit.photometry.conditional\_lf\_integrals module
+==================================================
+
+.. automodule:: lfkit.photometry.conditional_lf_integrals
+   :members:
+   :show-inheritance:
+   :undoc-members:
diff --git a/docs/api/lfkit.photometry.conditional_lf_models.rst b/docs/api/lfkit.photometry.conditional_lf_models.rst
@@ -0,0 +1,7 @@
+lfkit.photometry.conditional\_lf\_models module
+===============================================
+
+.. automodule:: lfkit.photometry.conditional_lf_models
+   :members:
+   :show-inheritance:
+   :undoc-members:
diff --git a/docs/api/lfkit.photometry.rst b/docs/api/lfkit.photometry.rst
@@ -8,6 +8,8 @@ Submodules
    :maxdepth: 2
 
    lfkit.photometry.catalog_completeness
+   lfkit.photometry.conditional_lf_integrals
+   lfkit.photometry.conditional_lf_models
    lfkit.photometry.lf_integrals
    lfkit.photometry.lf_parameter_models
    lfkit.photometry.lf_redshift_density

diff --git a/docs/examples/catalog_completeness_examples.rst b/docs/examples/catalog_completeness_examples.rst
@@ -2,8 +2,8 @@
    :alt: LFKit logo
    :width: 50px
 
-|lfkitlogo| Catalog completeness examples
-=========================================
+|lfkitlogo| Catalog completeness
+================================
 
 This page shows how to use :class:`lfkit.LuminosityFunction` to compute
 observed and missing galaxy number densities for a magnitude-limited catalog.