[ci skip] update dev list and fix docs warnings

pmocz · pmocz · commit ded8b1b04d5a · 2025-03-05T15:53:20.000-05:00
diff --git a/binary/test_suite/evolve_both_stars/README.rst b/binary/test_suite/evolve_both_stars/README.rst
@@ -10,28 +10,28 @@ This test case has 1 part. Click to see a larger version of a plot.
 
 * Part 1 (``inlist_project``) loads a 1 Msun and a 0.8 Msun zero-age main sequence models. The binary system has an initial period of 0.5 day, and is evolved until the Roche Lobe overflow indicator (R - Rlobe)/Rlobe  is greater than the default 0.0 value of ``accretor_overflow_terminate``:
 
-|br|
+
 Binary period Roche Lobe OverFlow mass transfer:
 
 .. image:: ../../../binary/test_suite/evolve_both_stars/docs/grid_001314.svg
    :width: 100%
 
 
-|br|
+
 Abundance and power generated by star 1:
 
 .. image:: ../../../binary/test_suite/evolve_both_stars/docs/profile_s1_001314.svg
    :width: 100%
 
 
-|br|
+
 Abundance and power generated by star 12:
 
 .. image:: ../../../binary/test_suite/evolve_both_stars/docs/profile_s2_001314.svg
    :width: 100%
 
 
-|br|
+
 pgstar commands used for the binary and star1 plots above:
 
 .. code-block:: console
@@ -234,7 +234,7 @@ pgstar commands used for the binary and star1 plots above:
  / ! end of pgstar namelist
 
 
-|br|
+
 pgstar commands used for the star2 plot above:
 
 .. code-block:: console
diff --git a/binary/test_suite/jdot_gr_check/README.rst b/binary/test_suite/jdot_gr_check/README.rst
@@ -21,14 +21,12 @@ This test case has 1 part. Click to see a larger version of a plot.
   terminate due to beginning of RLO
 
 
-|br|
 Binary period and separation history:
 
 .. image:: ../../../binary/test_suite/jdot_gr_check/docs/grid_000232.svg
    :width: 100%
 
 
-|br|
 pgstar commands used for the plot above:
 
 .. code-block:: console
diff --git a/binary/test_suite/jdot_ls_check/README.rst b/binary/test_suite/jdot_ls_check/README.rst
@@ -14,7 +14,7 @@ This test case has 1 part. Click to see a larger version of a plot.
    :width: 100%
 
 
-|br|
+
 pgstar commands used for the plot above:
 
 .. code-block:: console
diff --git a/binary/test_suite/jdot_ml_check/README.rst b/binary/test_suite/jdot_ml_check/README.rst
@@ -19,22 +19,22 @@ This test case has 1 part. Click to see a larger version of a plot.
    error in separation    7.0519985646485173D-05
 
 
-|br|
+
 Binary period and separation history:
 
 .. image:: ../../../binary/test_suite/jdot_ml_check/docs/grid_000891.svg
    :width: 100%
 
 
-|br|
+
 Abundance and power profiles of star 1 at termination:
 
 .. image:: ../../../binary/test_suite/jdot_ml_check/docs/profile_s1_000891.svg
    :width: 100%
 
 
 
-|br|
+
 pgstar commands used for the binary and star1 plots above:
 
 .. code-block:: console
diff --git a/binary/test_suite/star_plus_point_mass/README.rst b/binary/test_suite/star_plus_point_mass/README.rst
@@ -11,28 +11,28 @@ This test case has 1 part. Click to see a larger version of a plot.
 * Part 1 (``inlist_project``) loads a pre-built 5 Msun zero-age main sequence model as the donor and a 10 Msun point mass as the companion. The binary system has an initial period of 1 day, and is evolved until the central hydrogen mass fraction of the donor drops below 1e-2. Compare the evolutions bewlow with those in :ref:`star_plus_point_mass_explicit_mdot`.
 
 
-|br|
+
 Binary period versus model number:
 
 .. image:: ../../../binary/test_suite/star_plus_point_mass/docs/track1_000310.svg
    :width: 100%
 
 
-|br|
+
 Binary separation versus model number:
 
 .. image:: ../../../binary/test_suite/star_plus_point_mass/docs/track2_000310.svg
    :width: 100%
 
 
-|br|
+
 Kippenhang diagram of the mass losing donar:
 
 .. image:: ../../../binary/test_suite/star_plus_point_mass/docs/kipp_000310.svg
    :width: 100%
 
 
-|br|
+
 pgstar commands used for the plots above:
 
 .. code-block:: console
diff --git a/binary/test_suite/star_plus_point_mass_explicit_mdot/README.rst b/binary/test_suite/star_plus_point_mass_explicit_mdot/README.rst
@@ -10,28 +10,28 @@ This test case has 1 part. Click to see a larger version of a plot.
 
 * Part 1 (``inlist_project``) loads a pre-built 5 Msun zero-age main sequence model as the donor and a 10 Msun point mass as the companion. The binary system has an initial period of 1 day, and is evolved until the central hydrogen mass fraction of the donor drops below 1e-2. Compare the evolutions bewlow with those in :ref:`star_plus_point_mass`.
 
-|br|
+
 Binary period versus model number:
 
 .. image:: ../../../binary/test_suite/star_plus_point_mass_explicit_mdot/docs/track1_000565.svg
    :width: 100%
 
 
-|br|
+
 Binary separation versus model number:
 
 .. image:: ../../../binary/test_suite/star_plus_point_mass_explicit_mdot/docs/track2_000565.svg
    :width: 100%
 
 
-|br|
+
 Kippenhang diagram of the mass losing donar:
 
 .. image:: ../../../binary/test_suite/star_plus_point_mass_explicit_mdot/docs/kipp_000565.svg
    :width: 100%
 
 
-|br|
+
 pgstar commands used for the plots above:
 
 .. code-block:: console
diff --git a/docs/source/about.rst b/docs/source/about.rst
@@ -109,17 +109,16 @@ Developers
 * `Earl Bellinger <https://earlbellinger.com/>`__
 * `Lars Bildsten <http://www.kitp.ucsb.edu/bildsten/>`__
 * `Matteo Cantiello <http://www.matteocantiello.com/>`__
-* Matthias Fabry
-* Ebraheem Farag
-* Eoin Farrell
+* `Matthias Fabry <https://github.com/matthiasfabry>`__
+* `Ebraheem Farag <https://github.com/Debraheem>`__
 * `Jared Goldberg <https://jaredagoldberg.wordpress.com/>`__
 * `Meridith Joyce <http://www.meridithjoyce.com/>`__
 * `Pablo Marchant <https://orlox.github.io/>`__
 * `Philip Mocz <https://pmocz.github.io/>`__
 * `Joey Mombarg <https://jmombarg.github.io/PersonalWebsite/index.html>`__
 * `Mathieu Renzo <https://www.as.arizona.edu/~mrenzo/>`__
 * `Radek Smolec <https://www.camk.edu.pl/en/staff/smolec/>`__
-* Anne Thoul
+* `Anne Thoul <https://www.linkedin.com/in/anne-thoul-b8279853>`__
 * `Frank Timmes <http://cococubed.com/>`__
 * `Rich Townsend <http://www.astro.wisc.edu/~townsend>`__
 * `Bill Wolf <http://wmwolf.github.io/>`__
@@ -133,6 +132,7 @@ Past Developers
 * `Falk Herwig <http://www.astro.uvic.ca/~fherwig/>`__
 * `Adam Jermyn <http://adamjermyn.com/>`__
 * `Josiah Schwab <https://yoshiyahu.org/>`__
+* `Eoin Farrell <https://scholar.google.es/citations?user=Shv2DncAAAAJ&hl=es>`__`
 
 Other Code Contributors
 -----------------------
diff --git a/docs/source/using_mesa/best_practices.rst b/docs/source/using_mesa/best_practices.rst
@@ -196,7 +196,6 @@ and you should see a pgstar window appear on your screen:
 .. image:: grid4_000322.svg
    :width: 100%
 
-|br| |br|
 
 Explore Physics Variations
 --------------------------
@@ -229,9 +228,9 @@ Change the nuclear reaction network
 ``new_net_name`` = ``pp_and_cno_extras.net`` (this test suite case), ``basic.net`` (default), ``approx21.net``, and ``mesa_49.net``.
 
 1) Are all the reported values still within their tolerances at the end of a run?
-|br|
+
 2) Are the results for the growth of the convective core mass, HR diagram, and final hydrogen profile the same?
-|br|
+
 3) Why are the results the same or different?
 
 
diff --git a/star/test_suite/twin_studies/README.rst b/star/test_suite/twin_studies/README.rst
@@ -17,7 +17,6 @@ Star 1, with overshooting, reaches the ending age in 80 steps:
 .. image:: ../../../star/test_suite/twin_studies/docs/star1000080.svg
    :width: 100%
 
-|br| |br|
 Star 2, without overshooting, reaches the ending age in 273 steps. Star 2 is further along
 in its evolutionary path as might be expected without the extra fuel provided to the
 core by overshooting:
@@ -49,7 +48,6 @@ for star 1:
 
  / ! end of pgstar namelist
 
-|br|
 and for star 2:
 
 .. code-block:: console
diff --git a/star/test_suite/wd_c_core_ignition/README.rst b/star/test_suite/wd_c_core_ignition/README.rst
@@ -18,18 +18,18 @@ This test case has 2 parts. Click to see a larger version of a plot.
 
 .. image:: ../../../star/test_suite/wd_c_core_ignition/docs/track1_000747.svg
 
-|br|
+
 Central density and temperature evolution:
 
 .. image:: ../../../star/test_suite/wd_c_core_ignition/docs/trhoc_000747.svg
 
-|br|
+
 Convective and burn history
 
 .. image:: ../../../star/test_suite/wd_c_core_ignition/docs/kipp_000747.svg
 
 
-|br|
+
 pgstar commands used for the Part 1 plot above:
 
 .. code-block:: console
@@ -63,7 +63,7 @@ pgstar commands used for the Part 1 plot above:
  / ! end of pgstar namelist
 
 
-|br|
+
 pgstar commands used for the Part 2 plots above:
 
 .. code-block:: console
diff --git a/star/test_suite/wd_cool_0.6M/README.rst b/star/test_suite/wd_cool_0.6M/README.rst
@@ -14,13 +14,13 @@ This test case has 1 part. Click to see a larger version of a plot.
    :width: 100%
 
 
-|br|
+
 The evolution then commences with element diffusion activated, and the run terminates when the central temperature drops below 1e6 K:
 
 .. image:: ../../../star/test_suite/wd_cool_0.6M/docs/Grid2000578.svg
 
 
-|br|
+
 pgstar commands used for the plots above:
 
 .. code-block:: console
diff --git a/star/test_suite/wd_diffusion/README.rst b/star/test_suite/wd_diffusion/README.rst
@@ -20,7 +20,7 @@ This test case has 1 part. Click to see a larger version of a plot.
    :width: 100%
 
 
-|br|
+
 pgstar commands used for the plots above:
 
 .. code-block:: console
diff --git a/star/test_suite/wd_he_shell_ignition/README.rst b/star/test_suite/wd_he_shell_ignition/README.rst
@@ -8,28 +8,28 @@ This test case checks the ignition of a helium layer in an accreting in a 0.96 |
 
 This test case has 1 part. Click to see a larger version of a plot.
 
-* Part 1 (``inlist_he_shell_ignition``) loads 'co_wd_0.96M.mod', a 0.96 |Msun| carbon-oxygen white dwarf with a helium layer and then a hydrogen layer. The model is from a 6 |Msun| ZAMS progenitor with :ref:`make_co_wd` in r13718. Pure helium then accretes onto the hydrogen surface at a rate of 1e-9 |Msun|/yr. The helium layer ignites as the total mass approachess 1.36 |Msun|, and the run terminates when the helium burning luminosity first exceeds 1e11 |Lsun||:
+* Part 1 (``inlist_he_shell_ignition``) loads 'co_wd_0.96M.mod', a 0.96 |Msun| carbon-oxygen white dwarf with a helium layer and then a hydrogen layer. The model is from a 6 |Msun| ZAMS progenitor with :ref:`make_co_wd` in r13718. Pure helium then accretes onto the hydrogen surface at a rate of 1e-9 |Msun|/yr. The helium layer ignites as the total mass approachess 1.36 |Msun|, and the run terminates when the helium burning luminosity first exceeds 1e11 |Lsun|:
 
 
 .. image:: ../../../star/test_suite/wd_he_shell_ignition/docs/track1_000922.svg
    :width: 100%
 
-|br|
+
 The initial hydrogen burns as its pushed deeper into the model by accretion. The initial helium layer and the accreted helium
 thus merge to form a single helium layer. This single helium layer ignites at it is pushed to higher densities and temperatures
 by the continued accretion:
 
 .. image:: ../../../star/test_suite/wd_he_shell_ignition/docs/profile_000922.svg
    :width: 100%
 
-|br|
+
 Temperature and density profile at ignition:
 
 .. image:: ../../../star/test_suite/wd_he_shell_ignition/docs/trho_000922.svg
    :width: 100%
 
 
-|br|
+
 pgstar commands used for the plots above:
 
 .. code-block:: console
diff --git a/star/test_suite/wd_stable_h_burn/README.rst b/star/test_suite/wd_stable_h_burn/README.rst
@@ -15,7 +15,7 @@ This test case has 1 parts. Click to see a larger version of a plot.
    :width: 100%
 
 
-|br|
+
 pgstar commands used for the plots above:
 
 .. code-block:: console
