diff --git a/examples/tutorials/visualising_the_results.ipynb b/examples/tutorials/visualising_the_results.ipynb
index 83e445b6ebb7556c900a7f5752e48c191b098b34..d839005f34ef881f532c5099017b44273d5be3bf 100644
--- a/examples/tutorials/visualising_the_results.ipynb
+++ b/examples/tutorials/visualising_the_results.ipynb
@@ -35,8 +35,8 @@
     "\n",
     "# specify injection parameters\n",
     "injection_parameters = dict(\n",
-    "mass_1=36.,                          # source frame (non-redshifted) primary mass (solar masses)\n",
-    "mass_2=29.,                          # source frame (non-redshifted) secondary mass (solar masses)\n",
+    "mass_1=36.,                          # detector frame (redshifted) primary mass (solar masses)\n",
+    "mass_2=29.,                          # detector frame (redshifted) secondary mass (solar masses)\n",
     "a_1=0.4,                             # primary dimensionless spin magnitude\n",
     "a_2=0.3,                             # secondary dimensionless spin magnitude\n",
     "tilt_1=0.5,                          # polar angle between primary spin and the orbital angular momentum (radians)\n",
@@ -236,7 +236,6 @@
   {
    "cell_type": "markdown",
    "metadata": {
-    "collapsed": false,
     "pycharm": {
      "name": "#%% md\n"
     }
@@ -266,9 +265,7 @@
   },
   {
    "cell_type": "markdown",
-   "metadata": {
-    "collapsed": false
-   },
+   "metadata": {},
    "source": [
     "Again, notice that the plot is saved as a \"waveform.png\" in the output dir.\n",
     "\n",
@@ -277,7 +274,25 @@
    ]
   }
  ],
- "metadata": {},
+ "metadata": {
+  "kernelspec": {
+   "display_name": "Python 3",
+   "language": "python",
+   "name": "python3"
+  },
+  "language_info": {
+   "codemirror_mode": {
+    "name": "ipython",
+    "version": 3
+   },
+   "file_extension": ".py",
+   "mimetype": "text/x-python",
+   "name": "python",
+   "nbconvert_exporter": "python",
+   "pygments_lexer": "ipython3",
+   "version": "3.8.8"
+  }
+ },
  "nbformat": 4,
  "nbformat_minor": 2
 }