Back to development: 1.3

Chandra-MARX · Nov 6, 2020 · c1acbe2 · c1acbe2
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diff --git a/CHANGES.rst b/CHANGES.rst
@@ -1,3 +1,21 @@
+1.3 (unreleased)
+----------------
+
+New Features
+^^^^^^^^^^^^
+
+
+API Changes
+^^^^^^^^^^^
+
+
+Bug fixes
+^^^^^^^^^
+
+Other changes and additions
+^^^^^^^^^^^^^^^^^^^^^^^^^^^
+
+
 1.2 (06-Nov-2020)
 -----------------
 
@@ -64,7 +82,7 @@ API Changes
   for subclasses). [#202]
 
 - `~marxs.optics.RandomGaussianScatter` and `~marxs.optics.Scatter` now expect
-  angular quantities instead of plai floats. [#216]
+  angular quantities instead of plain floats. [#216]
 
 
 Bug fixes

diff --git a/setup.cfg b/setup.cfg
@@ -17,7 +17,7 @@ auto_use = True
 
 [metadata]
 name = marxs
-version = 1.2
+version = 1.3dev
 description = Multi Architecture Raytracer for X-ray satellites
 long_description = MARXS (Multi-Architecture-Raytrace-Xraymission-Simulator) is a toolsuite to simulate the performance X-ray observatories. It is primarily aimed at astronomical X-ray satellites and sounding rocket payloads, but can be used to ray-trace experiments in the laboratory as well. MARXS performs Monte-Carlo ray-trace simulations from a source (astronomical or lab) through a collection of optical elements such as mirrors, baffles, and gratings to a detector.
 author = MIT / H. M. Günther