minor change to clarify sections of notebook

examples/test_coordinate.ipynb

@@ -20,6 +20,9 @@
     "- Example source galaxies for galaxy clusters from a [Summer School](https://github.com/oguri/wlcluster_tutorial) taught by Masamune Oguri (pixel coordinate system)\n",
     "- HSC Y3 source galaxies with shears post processed by Tomomi Sunayama (sky coordinate system)\n",
     "\n",
+    "We also \n",
+    "- Compare the explicit calculation of a shear profile on the HSC Y3 source galaxies against a profile produced from `CLMM`. \n",
+    "\n",
     "Before running this notebook, you will need to download some data.  The data is available through a [dropbox link](https://www.dropbox.com/scl/fo/dwsccslr5iwb7lnkf8jvx/AJkjgFeemUEHpHaZaHHqpAg?rlkey=efbtsr15mdrs3y6xsm7l48o0r&st=xb58ap0g&dl=0)\n",
     "\n",
     "First, create a directory where you want to put the example data, e.g.\n",
@@ -695,7 +698,7 @@
    "id": "c06de4dd-be05-4b16-9d99-bfab31ee04c9",
    "metadata": {},
    "source": [
-    "## Example explicit lensing measurement (not with CLMM)\n",
+    "## Example explicit lensing profile measurement comparison with CLMM profile\n",
     "\n",
     "Here, we use the example HSC Y3 dataset to explicitly measure the lensing signal without using CLMM for comparison.  Note, we need to still define a cosmology to calculate comoving distances."
    ]