finish off some final todos

Author: nmdickson

docs/source/fitting.rst

@@ -328,6 +328,7 @@ normalized probability distribution is obtained.
 The measured timing solution is then interpolated onto this distribution,
 computing a final likelihood value, for this pulsar. All pulsars in the cluster
 have their likelihoods summed in the usual manner.
+
 .. TODO DM stuff
 
 

docs/source/ref/api.rst

@@ -4,7 +4,7 @@ API
 
 This page details the methods and classes provided by the ``GCfit`` module.
 
-TODO seems like the autogen is duplicating all the methods in classes
+.. TODO this imaage needs to be updated since nested classes were split off
 
 .. image:: package-structure.png
 

fitter/core/data.py

@@ -645,6 +645,7 @@ def _determine_likelihoods(self):
 
 # TODO The units are *quite* incomplete in Model (10)
 # TODO would be cool to get this to work with limepy's `sampling`
+# TODO what attributes should be documented?
 
 class Model(lp.limepy):
     r'''Wrapper class around a LIMEPY model, including mass function evolution
@@ -666,7 +667,8 @@ class Model(lp.limepy):
     theta : dict or list
         The model input parameters. Must either be a dict, or a full list of
         all parameters, in the exact same order as `DEFAULT_INITIALS`.
-        See {{TODO docs}} for explanation of all possible input parameters.
+        See package background documentation for explanation of all possible
+        input parameters.
 
     observations : Observations, optional
         The `Observations` instance corresponding to this cluster. While not
@@ -685,8 +687,6 @@ class Model(lp.limepy):
     {BH,NS,WD}_Nj : astropy.Quantity
         Black hole, neutron star or white dwarf total bin number (Mj / mj)
 
-    # TODO none of the other important attributes were documented
-
     Notes
     -----
     The IMF of the model is defined using a three-component broken power law,