Tutorial typo fix

docs/source/tutorials/tutorial_MIRI_contrast_analyses.ipynb

@@ -1659,7 +1659,7 @@
    "metadata": {},
    "source": [
     "---\n",
-    "The results obtained here can be directly compared to the [JWST Early Release Science (ERS) coronagraphic observations of the super-Jupiter exoplanet HIP 65426b](https://iopscience.iop.org/article/10.3847/2041-8213/acd93e), published by Aarynn Carter et al. Specifically, we find in the tutorial an absolute magnitude (relative to Vega) of 13.794±0.1870, compared to the paper's report of 14.705±0.182. Differences can be due to various updates in the JWST pipeline (notably an update to MIRI flux calibration) and the spaceKLIP algorithm. Additionally, note that the ERS paper employs a different error analysis method. \n",
+    "The results obtained here can be directly compared to the [JWST Early Release Science (ERS) coronagraphic observations of the super-Jupiter exoplanet HIP 65426b](https://iopscience.iop.org/article/10.3847/2041-8213/acd93e), published by Aarynn Carter et al. Specifically, we find in the tutorial an apparent magnitude (relative to Vega) of 13.794±0.1870, compared to the paper's report of 14.705±0.182. Differences can be due to various updates in the JWST pipeline (notably an update to MIRI flux calibration) and the spaceKLIP algorithm. Additionally, note that the ERS paper employs a different error analysis method. \n",
     "\n",
     "Congratulations on completing the analysis on HIP 65426 b with spaceKLIP!"
    ]

docs/source/tutorials/tutorial_NIRCam_contrast_analyses.ipynb

@@ -1971,10 +1971,16 @@
    "metadata": {},
    "source": [
     "---\n",
-    "The results obtained here can be directly compared to the [JWST Early Release Science (ERS) coronagraphic observations of the super-Jupiter exoplanet HIP 65426b](https://iopscience.iop.org/article/10.3847/2041-8213/acd93e), published by Aarynn Carter et al. Specifically, we find in the tutorial an absolute magnitude (relative to Vega) of 15.393±0.0133, compared to the paper's report of 15.467±0.078, consistent within 1-sigma of the tutorial values. Differences can be due to various updates in the JWST pipeline and the spaceKLIP algorithm. Additionally note that the ERS paper employs a different error analysis method. \n",
+    "The results obtained here can be directly compared to the [JWST Early Release Science (ERS) coronagraphic observations of the super-Jupiter exoplanet HIP 65426b](https://iopscience.iop.org/article/10.3847/2041-8213/acd93e), published by Aarynn Carter et al. Specifically, we find in the tutorial an apparent magnitude (relative to Vega) of 15.393±0.0133, compared to the paper's report of 15.467±0.078, consistent within 1-sigma of the tutorial values. Differences can be due to various updates in the JWST pipeline and the spaceKLIP algorithm. Additionally note that the ERS paper employs a different error analysis method. \n",
     "\n",
     "Congratulations on completing the analysis on HIP 65426 b with spaceKLIP!"
    ]
+  },
+  {
+   "cell_type": "markdown",
+   "id": "8522ee5e",
+   "metadata": {},
+   "source": []
   }
  ],
  "metadata": {