Update pixel area map notebook links to Jahia and HDox versions

tddesjardins · Jul 1, 2019 · 69deabf · 69deabf
1 parent 95f95be
commit 69deabf
Showing 1 changed file with 4 additions and 4 deletions.
diff --git a/acs_pixel_area_maps/acs_pixel_area_maps.ipynb b/acs_pixel_area_maps/acs_pixel_area_maps.ipynb
@@ -24,7 +24,7 @@
     "\n",
     "A pixel area map (PAM), which is an image where each pixel value describes that pixel's area on the sky relative to the native plate scale, is used for this correction. The distortion corrections applied by both AstroDrizzle and the PAMs include observation-specific corrections (e.g., velocity distortion). For the best results, users are advised to create a PAM for each observation individually.\n",
     "\n",
-    "To transform a distorted FLT/FLC image so that it is suitable for photometry, users must multiply the image by the PAM and divide the result by the exposure time so that the image has units of electrons/second. After this transformation, the information on the [ACS Zeropoints](http://www.stsci.edu/hst/acs/analysis/zeropoints/) page can be used to convert flux measurements into physical units.\n",
+    "To transform a distorted FLT/FLC image so that it is suitable for photometry, users must multiply the image by the PAM and divide the result by the exposure time so that the image has units of electrons/second. After this transformation, the information on the [ACS Zeropoints](http://www.stsci.edu/hst/instrumentation/acs/data-analysis/zeropoints) page can be used to convert flux measurements into physical units.\n",
     "\n",
     "### This tutorial will show you how to...\n",
     "\n",
@@ -132,7 +132,7 @@
    "source": [
     "## File Information\n",
     "***\n",
-    "The structure of the fits files from ACS may be different depending on what kind of observation was made. For more information, refer to Section <a class=\"divlink\" href=\"http://www.stsci.edu/hst/acs/documents/handbooks/currentDHB/acs_Ch23.html\">Section 2.2</a> of the ACS Data Handbook.\n",
+    "The structure of the fits files from ACS may be different depending on what kind of observation was made. For more information, refer to Section 2.2 of the [ACS Data Handbook](http://www.stsci.edu/files/live/sites/www/files/home/hst/instrumentation/acs/documentation/other-documents/_documents/acs_dhb.pdf).\n",
     "\n",
     "#### FLT Files (WFC-Specific)\n",
     "\n",
@@ -261,7 +261,7 @@
    "source": [
     "### For more help:\n",
     "\n",
-    "More details may be found on the [ACS website]() and in the [ACS Instrument]() and [Data Handbooks](). Geometric Distortion information can be found in [Section 5.6.4](http://www.stsci.edu/hst/acs/documents/handbooks/current/c05_imaging7.html#357374) of the ACS Instrument Handbook.\n",
+    "More details may be found on the [ACS website](http://www.stsci.edu/hst/instrumentation/acs) and in the [ACS Instrument](https://hst-docs.stsci.edu/display/ACSIHB) and [Data Handbooks](http://www.stsci.edu/files/live/sites/www/files/home/hst/instrumentation/acs/documentation/other-documents/_documents/acs_dhb.pdf). Geometric Distortion information can be found in [Section 5.6.4](https://hst-docs.stsci.edu/display/ACSIHB/5.6+ACS+Point+Spread+Functions) and [Section 10.4](https://hst-docs.stsci.edu/display/ACSIHB/10.4+Geometrical+Distortion+in+the+ACS) of the ACS Instrument Handbook.\n",
     "\n",
     "Please visit the [HST Help Desk](http://hsthelp.stsci.edu). Through the help desk portal, you can explore the *HST* Knowledge Base and request additional help from experts."
    ]
@@ -283,7 +283,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.5.6"
+   "version": "3.6.7"
   }
  },
  "nbformat": 4,