Fix broken image link in acs_saturation_trails.ipynb

notebooks/ACS/acs_saturation_trails/acs_saturation_trails.ipynb

@@ -29,9 +29,10 @@
     "\n",
     "However, accurate relative photometry can be obtained as long as a large enough aperture is selected to contain the spilled flux ([ACS ISR 2004-01](http://www.stsci.edu/files/live/sites/www/files/home/hst/instrumentation/acs/documentation/instrument-science-reports-isrs/_documents/isr0401.pdf)). While one could simply use a larger circular aperture, that may introduce error when working with a crowded field (where bright stars are often located).\n",
     "\n",
-    "Here we present a method to identify and perform photometry on saturated sources by defining a custom aperture that is a combination of a standard 0.5\" arcsecond circular aperture and the pixels affected by saturation trails. This method has been tested on ACS/WFC observations of 47 Tuc in the F660W band. The plot below shows the results of using this alternative method to recover flux.\n",
+    "Here we present a method to identify and perform photometry on saturated sources by defining a custom aperture that is a combination of a standard 0.5\" arcsecond circular aperture and the pixels affected by saturation trails. This method has been tested on ACS/WFC observations of 47 Tuc in the F606W band. The plot below shows the results of using this alternative method to recover flux.\n",
+    "\n",
+    "<img src=photometry_recovery.png width =\"900\" title=\"\" alt=\"\">\n",
     "\n",
-    "![title](photometry_plot.png)\n",
     "\n",
     "### This tutorial will show you how to...\n",
     "\n",
@@ -1193,7 +1194,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.9.13"
+   "version": "3.8.12"
   }
  },
  "nbformat": 4,