diff --git a/CHANGES.txt b/CHANGES.txt
index 21f9eae..9aa2567 100644
--- a/CHANGES.txt
+++ b/CHANGES.txt
@@ -1,6 +1,14 @@
 Changelog
 ---------
 
+Version 0.1.0
+
+* Fixed `get_surface()` that demand all the z points.
+* Fixed `get_nearest_water()` to loop over all the points until actually finds
+  water.
+* Added `get_nearest_series()` when finding wanter is not an issue (much faster
+  than `get_nearest_water()`.
+
 Version 0.0.1
 
 * First release (Factored out from utilities)
diff --git a/README.rst b/README.rst
index ee614ff..70fe41b 100644
--- a/README.rst
+++ b/README.rst
@@ -14,5 +14,14 @@ TARDIS is a collection of function for iris
 TARDIS (Time and Relative Dimension(s) in Space) is module to travel an
 `iris <http://scitools.org.uk/iris/docs/latest/index.html>`__ cube.
 
-No docs at the moment...
-`Move along... <https://ocefpaf.github.io/python4oceanographers/blog/2015/06/29/tardis/>`__
+No docs at the moment... `Move along! <https://ocefpaf.github.io/python4oceanographers/blog/2015/06/29/tardis/>`__
+
+Depending on which model is used, the horizontal coordinate of the output data
+may be on a regular, curvilinear, or unstructured (e.g., triangular) grid,
+while the vertical coordinate may be on a uniform or stretched grid with a
+number of different possibilities (e.g., sigma, sigma-over-z, s-coordinate,
+isopycnal).  Ocean modelers spend way to much time on data manipulation tasks
+just to read the data!!!
+
+Tardis complements the iris cube with some extra methods to make that task
+even easier.