(docs) fix broken links [skip ci]

danieljprice · Jan 31, 2024 · 7c15728 · 7c15728
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diff --git a/docs/developer-guide/stable.rst b/docs/developer-guide/stable.rst
@@ -2,7 +2,7 @@ How to use download and use stable code releases
 ================================================
 
 The master branch of phantom develops rapidly, but if you want to only
-:doc:`stable versions of phantom <releasenotes>`, the best way is to use
+:doc:`stable versions of phantom <../releasenotes>`, the best way is to use
 the \`stable’ code branch from the git repository. **Nobody has
 permission** to push directly to the stable branch, it must be updated
 via pull request, so it **cannot** be inadvertently broken

diff --git a/docs/developer-guide/staging.rst b/docs/developer-guide/staging.rst
@@ -5,7 +5,7 @@ Procedure is:
 
 - set the version number in phantom/build/Makefile
 - set the version number in phantom/docs/conf.py
-- update the :doc:`release notes <releasenotes>`
+- update the :doc:`release notes <../releasenotes>`
 - use git to tag the code version for the release
 
 ::

diff --git a/docs/examples/disc.rst b/docs/examples/disc.rst
@@ -138,7 +138,7 @@ The above procedure prints a .discparams file (in the above example would be
 called disc.discparams) that contains some of the parameters used to
 initialise the disc setup.
 
-For a circumbinary disc the equation of state is set to a vertically isothermal equation of state (ieos=3) where the radius is taken with respect to *the coordinate origin*. See :doc:`Equations of state available in Phantom <eos>`
+For a circumbinary disc the equation of state is set to a vertically isothermal equation of state (ieos=3) where the radius is taken with respect to *the coordinate origin*. See :doc:`Equations of state available in Phantom </physics/eos>`
 
 check the .in file and proceed to run phantom
 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
@@ -181,7 +181,7 @@ which produces::
   secondary mass          :    1.00
   mass ratio              :    1.00
 
-For a circumprimary disc the equation of state is set to ieos=6, such that the radius is taken with respect to the first sink particle in the simulation. See :doc:`Equations of state available in Phantom <eos>`
+For a circumprimary disc the equation of state is set to ieos=6, such that the radius is taken with respect to the first sink particle in the simulation. See :doc:`Equations of state available in Phantom <physics/eos>`
 
 The Farris et al. (2014) :doc:`equation of state <eos>` (ieos=14 for a binary or ieos=13 if there are more than two stars) is also useful for a flyby simulation if one does not want to have excessively cold material around the secondary
 

diff --git a/docs/getting-started/running-first-calculation.rst b/docs/getting-started/running-first-calculation.rst
@@ -153,7 +153,7 @@ For the Sedov example shown above, there’s even an exact solution included in
 
 .. important::
    If you have v2.x or earlier of splash,
-   type ssplash instead of splash to read :doc:`the phantom native binary format<dumpfile>`.
+   type ssplash instead of splash to read :doc:`the phantom native binary format</user-guide/dumpfile>`.
 
 The .ev files, which are just ascii files containing global quantities as a function of time::
 

diff --git a/docs/developer-guide/data-curation.rst → docs/user-guide/data-curation.rst b/docs/developer-guide/data-curation.rst → docs/user-guide/data-curation.rst