Edited README to include epsilon scaling
@@ -10,7 +10,7 @@ Overview
**Modules** atmesc
stellar
**Approx. runtime** 49 seconds
-**Source code** `GitHub <https://github.com/VirtualPlanetaryLaboratory/vplanet-private/tree/master/examples/venus_ocean>`_
+**Source code** `GitHub <https://github.com/VirtualPlanetaryLaboratory/vplanet-private/tree/master/examples/VenusWaterLoss>`_
=================== ============
Water loss on Venus from thermal processes.
@@ -37,3 +37,19 @@ Expected output
by the surface (right) as a function of time for three different initial
surface water inventories. The vertical dashed line is the Watson et al. (1981)
:cite:`Watson81` timescale for the complete desiccation of Venus.
+
+To run this example
+-------------------
+
+.. code-block:: bash
+
+ cd BolmontEps
+ vplanet vpl.in
+ python makeplot.py <pdf | png>
+
+.. figure:: EpsilonScaling.png
+ :width: 600px
+ :align: center
+
+ The scaling of the atmospheric escape efficiency for H2O based on the XUV flux
+ received by the planet as given by Bolmont (2016) :cite:`Bolmont16`.
