diff --git a/examples/demo_coordinate_system_datasets.ipynb b/examples/demo_coordinate_system_datasets.ipynb
index 4f8dc867c..8e4410271 100644
--- a/examples/demo_coordinate_system_datasets.ipynb
+++ b/examples/demo_coordinate_system_datasets.ipynb
@@ -10,6 +10,7 @@
     "\n",
     "Tested, modified, and documented by: Camille Avestruz, July 18, 2024\n",
     "\n",
+    "Reviewed by: Caio Lima de Oliveira, July 19, 2024\n",
     "\n",
     "This notebook illustrates the impact of having an incorrect coordinate system when calculating shear profiles.  The default coordinate system for `CLMM` is the euclidean/pixel coordinate system.  This is consistent with DC2 catalogs.  However, if we input a catalog that assumes a celestial (sky) coordinate system and use the default euclidean (pixel) coordinate system (or vice versa), the signal of shear around a cluster disappears because the signal essentially looks random.\n",
     "\n",