diff --git a/doc/sphinx/ApproxForTH.png b/doc/sphinx/ApproxForTH.png
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diff --git a/doc/sphinx/GibbsOrder.png b/doc/sphinx/GibbsOrder.png
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diff --git a/doc/sphinx/PMGvsMGUsupPress.png b/doc/sphinx/PMGvsMGUsupPress.png
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diff --git a/doc/sphinx/SteinbergGammarho.png b/doc/sphinx/SteinbergGammarho.png
new file mode 100644
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diff --git a/doc/sphinx/src/getting-started.rst b/doc/sphinx/src/getting-started.rst
index 6da789e70c..2e6c048aa2 100644
--- a/doc/sphinx/src/getting-started.rst
+++ b/doc/sphinx/src/getting-started.rst
@@ -9,9 +9,8 @@ At it's most basic, you can download and compile ``singularity-eos`` with:
 
   git clone --recursive git@github.com:lanl/singularity-eos.git
   cd singularity-eos
-  mkdir bin
-  cd bin
-  cmake -DSINGULARITY_FORCE_SUBMODULE_MODE=ON -DSINGULARITY_USE_FORTRAN=OFF ..
+  mkdir -p build && cd build
+  cmake -DSINGULARITY_FORCE_SUBMODULE_MODE=ON -DSINGULARITY_USE_FORTRAN=OFF -DSINGULARITY_BUILD_EXAMPLES=ON -DSINGULARITY_BUILD_TESTS=ON ..
   make -j
   make install # optional: install into directory defined via CMAKE_INSTALL_PREFIX
 
@@ -19,6 +18,26 @@ This will download ``singularity-eos`` with no optional dependencies and
 compile the capabilities available in that form. For more details, see
 :ref:`our build page <building>`.
 
+You can also run unit tests by calling
+
+.. code-block::
+
+  make test
+
+which should produce output confirming that several tests pass.
+
+Once compiled, you can quickly check your build/install by going to
+``build/example`` and running ``./get_sound_speed_press``. You should be
+able to see the following output:
+
+.. code-block::
+
+  The final values are:
+  rho = 0.987467
+  uu  = 0.00987467
+  P   = 0.0059248
+  cs  = 0.0979796
+
 If the library is in your include and lib paths (or you built it
 in-tree), you can include the ``eos`` part of the library with
 
diff --git a/doc/sphinx/src/models.rst b/doc/sphinx/src/models.rst
index e2db07f41b..c3517e7529 100644
--- a/doc/sphinx/src/models.rst
+++ b/doc/sphinx/src/models.rst
@@ -698,7 +698,7 @@ If the unitless user parameter :math:`b=\Gamma_0`, the Gruneisen parameter is of
 form where :math:`\Gamma_0 =` constant in compression. These two limitig cases are 
 shown in the figure below.
 
-.. image:: ../SteinbergGammarho.pdf
+.. image:: ../SteinbergGammarho.png
   :width: 500
   :alt: Figure: Demonstration of how the parameter b interpolated between two common approximations for Gamma
 
@@ -978,7 +978,7 @@ The first omitted term in the expansion inside the square brackets is :math:`\Ga
 in fact even better than the common approximation of replacing the full temperature on the Hugoniot with the temperature on the 
 isentrope, that is, the first term :math:`T_0 e^{\Gamma(\rho_0) \eta}`.
 
-.. image:: ../ApproxForTH.pdf
+.. image:: ../ApproxForTH.png
   :width: 500
   :alt: Figure: Different approximations for the temperature on the Hugoniot.
 
@@ -1018,7 +1018,7 @@ By expanding the MGUsup Hugoniot pressure into a power series in :math:`\eta` we
 
 In the figure below we have used :math:`M=20` with these coefficients and show how the divergence in the MGUsup pressure at :math:`\eta = \frac{1}{s}` is avoided in the PowerMG, making it more suitable for modeling high pressures.
 
-.. image:: ../PMGvsMGUsupPress.pdf
+.. image:: ../PMGvsMGUsupPress.png
   :width: 500
   :alt: Figure: Comparing Hugoniot pressure for PowerMG and MGUsup
 
diff --git a/doc/sphinx/src/python.rst b/doc/sphinx/src/python.rst
index 3add0268cb..651d4cd0ea 100644
--- a/doc/sphinx/src/python.rst
+++ b/doc/sphinx/src/python.rst
@@ -7,6 +7,10 @@ Singularity EOS provides Python bindings which can be enabled with the CMake
 ``SINGULARITY_BUILD_PYTHON`` option. They provide a 1:1 mapping of the C++ EOS
 types and give access to both scalar and vector functions.
 
+Where you build or install your python bindings to must be included in
+your python module search path. For example, if you do not install,
+this may be ``singularity-eos/build/python``.
+
 .. note::
 
    At this time, all Python bindings are host-only.
diff --git a/doc/sphinx/src/using-kpt.rst b/doc/sphinx/src/using-kpt.rst
index c4265603e2..acd8025da3 100644
--- a/doc/sphinx/src/using-kpt.rst
+++ b/doc/sphinx/src/using-kpt.rst
@@ -183,7 +183,7 @@ transportation rate from/to phases ``fromto[k]``, with ``k`` a phase transition
 in ``fromto``, "ij", is composed from the ``gibbs`` index of the "from" phase, :math:`i`, and the ``gibbs`` index of the "to" phase, 
 :math:`j`, as :math:`i*10+j`, and with a single digit integer, "x", interpreted as "0x".
 
-.. image:: ../GibbsOrder.pdf
+.. image:: ../GibbsOrder.png
   :width: 500
   :alt: Figure: How the phase transition index used in several arrays relate to the phase index in the  gibbsorder array.