[ci optional], tweak changelog, do full test

Author: Debraheem

docs/source/changelog.rst

@@ -89,18 +89,20 @@ The phase diagram for O/Ne separation comes from
 
 Massive Star test_suite Updates
 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+
 The ``12Msun_pre_ms_to_core_collapse``, ``20Msun_pre_ms_to_core_collapse``, and ``zams_to_cc_80``
 test_suites have each been updated and now fully evolve models at solar metallicities to core
 collapse while keeping their surface boundaries at tau = 1. The models offer a framework which
 has been tested to function with large reaction networks containing > 200 isotopes thanks to
- 'op_split_burn'. This updates includes the revival of the ``make_pre_ccsn_13bvn`` test_suite
+'op_split_burn'. This updates includes the revival of the ``make_pre_ccsn_13bvn`` test_suite
 as seen in section 6.9 of MESA IV.
 
 
 .. _Bug Fixes main:
 
 Bug Fixes
 ---------
+
 The ZAMS model data used to generate the initial model for simulations with
 ``create_pre_main_sequence_model = .false.`` and ``load_saved_model = .false.``
 had an issue where stars between 1.0 and 1.58 Msun would have a starting 
@@ -110,8 +112,8 @@ and now all pre-computed ZAMS models have a central hydrogen mass fraction very
 near 0.697.
 
 The ``fixed_Teff``, ``fixed_Tsurf``, ``fixed_Psurf``,  and ``fixed_Psurf_and_Tsurf``
-atmosphere options have been reimplemented, although we caution users that their
-implementation might conflict with mlt_option = ``TDC``.
+atmosphere options were removed in r15140. We have reimplemented them although we
+caution users that their implementation could conflict with ``mlt_option = 'TDC'``.
 
 Changes in r23.05.1
 ===================