Merge pull request #107 from joshwalawender/master

Update mkdocs config and PDF to include new examples section

manual/docs/changes.md

@@ -7,7 +7,7 @@
 * Python3 compatibility!
 * Improved installation procedure uses anaconda cloud
 * The 1D spectral extraction code now provides the user the ability to set the default aperture width.
-* Revamped documentation using mkdocs
+* Revamped documentation using mkdocs including the addition of an examples section.
 
 __Note__: This release of the DRP is only tested and supported on python 3.6+.  If you must use python 2, use the 2016 release of the DRP.  We encourage all users to use python 3 and we make the install of python 3 easy using anaconda python and the anaconda cloud (see the installation instructions).
 

manual/docs/generate_pdf

@@ -1 +1 @@
-pandoc -o MOSFIRE_DRP_Manual.pdf manual.md changes.md preface.md installing.md retrieve.md handle.md autodriver.md driver.md flats.md wavelengthYJH.md wavelengthK.md background.md rectify.md extract.md long2pos.md longslit.md headercomments.md hints.md
+pandoc -o MOSFIRE_DRP_Manual.pdf manual.md changes.md preface.md installing.md retrieve.md handle.md autodriver.md driver.md flats.md wavelengthYJH.md wavelengthK.md background.md rectify.md extract.md long2pos.md longslit.md headercomments.md hints.md example.md

manual/docs/hints.md

@@ -8,4 +8,4 @@ The output above shows that up to pixel 1015 the RMS was 0.27 Angstrom level, an
 
 ## Look at rectified_wave_stack files
 
-Look at rectified_wave_stack* files and make sure the night sky lines are vertical on the detector.
+Look at rectified_wave_stack* files and make sure the night sky lines are vertical on the detector.

manual/mkdocs.yml

@@ -21,3 +21,4 @@ pages:
         - 'Longslit Reductions': longslit.md
         - 'A Word About Header Comments': headercomments.md
         - 'Some Hints': hints.md
+        - 'Examples of Running the Pipeline': example.md