@@ -39,13 +39,15 @@ Model Partition Calibration is inspired by the paper:
 Radio interferometric calibration with SAGE, S Kazemi, S Yatawatta, S Zaroubi, P Lampropoulos, A G de Bruyn, L V E
 Koopmans, and J Noordam, Monthly Notices of the Royal Astronomical Society, 2011 vol. 414 (2) pp. 1656-1666.
 
+.. image:: ./Model_Partition_Calibration_View.png
+   :scale: 100 %
+
 In this code:
 
 - A single modelpartition is taken to be a vector composed of skycomponent, gaintable tuples.
 
-
 - The E step for a specific window is the sum of the window data model and the discrepancy between the observed data
-   and the summed modelpartitions.
+and the summed modelpartitions.
 
 - The M step for a specific window is the optimisation of the skymodel vector given the window data model. This involves fitting a skycomponent and fitting for the gain phases.
 
 
@@ -71,12 +71,6 @@ Calibration
 * Solve for complex gains: :py:mod:`processing_components.calibration.calibration.solve_gaintable`
 * Apply complex gains: :py:mod:`processing_components.calibration.operations.apply_gaintable`
 
-Model Partition Calibration
-===========================
-
-* Define model partition: :py:mod:`processing_components.calibration.modelpartition.create_modelpartition`
-* Solve model partition: :py:mod:`processing_components.calibration.modelpartition.solve_modelpartition`
-
 Coordinate transforms
 =====================