diff --git a/docs/pages/Model-Files.md b/docs/pages/Model-Files.md
index 03a0c5203e8e00e5ed6a4e08fd34defd3f8c7748..1e573cb77f3ce5b31da8417f320e745d351dd796 100644
--- a/docs/pages/Model-Files.md
+++ b/docs/pages/Model-Files.md
@@ -140,7 +140,7 @@ source-tree branches.
 How MFDs are intialized (or realized) depends on the presence and contents of `mfd-config.json` and
 `rate-tree.json` files. See the
 [magnitude frequency distributions](./Magnitude-Frequency-Distributions.md) page for details on
-these files and the types of MFDs supported in _nshmp-haz_. Note also the 
+these files and the types of MFDs supported in _nshmp-haz_.
 
 ## Rupture Sets
 
diff --git a/docs/pages/Source-Types.md b/docs/pages/Source-Types.md
index 67244fe9d8a865324bd391220e2e70117b01e6e3..fc6d2042ce951aa1b8662901e7c797e811df57ca 100644
--- a/docs/pages/Source-Types.md
+++ b/docs/pages/Source-Types.md
@@ -50,7 +50,6 @@ defines the bounds of the gridded seismicity source. A grid rupture set `mfd-tre
 defined inline and always points to a tree in a
 [`mfd-map`](./Magnitude-Frequency-Distributions.md#mfd-construction).
 
-
 ```json
 [
   {
@@ -106,7 +105,7 @@ some may contain depth values (intraslab sources), maximum magnitude caps, or ot
 spatial PDFs are the preferred approach to modeling regional rate variations, however it is also
 possible to define explicit MFDs at each grid node. To do so, the `spatial-pdf` member
 of a **rupture-sets.json** is replaced with `grid-mfds`. See
-`2018 CONUS NSHM > active-crust > grid-sources` for examples of both approaches. 
+`2018 CONUS NSHM > active-crust > grid-sources` for examples of both approaches.
 
 ## Zone Sources