records: update prescale example link for 2015 lumi

cernopendata/modules/fixtures/data/records/cms-detailed-luminosity-information.json

@@ -159,7 +159,7 @@
   },
   {
     "abstract": {
-      "description": "<p>CMS measures the luminosity using different luminometers (luminosity detectors) and algorithms. The luminometer giving the best value for each luminosity section is recorded in a 'normtag' file <a href=\"/record/1055/files/normtag_PHYSICS_2015.json\">normtag_PHYSICS_2015.json</a> that is used in the luminosity calculation.</p><p>The integrated luminosity for validated runs and luminosity sections of the 2015 public data (Run2015D) is available in <a href=\"/record/1055/files/Run2015Dlumi.txt\">Run2015Dlumi.txt</a>. (The integrated luminosity for validated runs and luminosity sections of all 2015 p-p data taking is available in <a href=\"/record/1055/files/2015lumi.txt\">2015lumi.txt</a>.)</p><p> For luminosity calculation, a detailed list of luminosity by lumi section is provided in <a href=\"/record/1055/files/2015lumibyls.csv\">2015lumibyls.csv</a> for the <a href=\"/record/14210\">list of validated runs</a> and lumi sections.</p><p>The uncertainty in the luminosity measurement of 2015 data should be considered as 1.6% (reference <a href=\"https://cds.cern.ch/record/2759951\">Precision luminosity measurement in proton-proton collisions at $\\sqrt{s} =$ 13 TeV in 2015 and 2016 at CMS</a>).</p><p>In your estimate for the integrated luminosity, check for which runs the trigger you have selected is active and sum the values for those runs. If you are using prescaled triggers, you can find the trigger prescale factors as shown in <a href=\"/record/5004\">the trigger examples</a>. The change of prescales (run, lumi section, index of prescales) is recorded in <a href=\"/record/1055/files/prescale2015.csv\">prescale2015.csv</a></p><p>Additional information on how to extract luminosity values using the <strong>brilcalc tool</strong> can be found in the <a href=\"/docs/cms-guide-luminosity-calculation\"> luminosity calculation guide</a>.</p>"
+      "description": "<p>CMS measures the luminosity using different luminometers (luminosity detectors) and algorithms. The luminometer giving the best value for each luminosity section is recorded in a 'normtag' file <a href=\"/record/1055/files/normtag_PHYSICS_2015.json\">normtag_PHYSICS_2015.json</a> that is used in the luminosity calculation.</p><p>The integrated luminosity for validated runs and luminosity sections of the 2015 public data (Run2015D) is available in <a href=\"/record/1055/files/Run2015Dlumi.txt\">Run2015Dlumi.txt</a>. (The integrated luminosity for validated runs and luminosity sections of all 2015 p-p data taking is available in <a href=\"/record/1055/files/2015lumi.txt\">2015lumi.txt</a>.)</p><p> For luminosity calculation, a detailed list of luminosity by lumi section is provided in <a href=\"/record/1055/files/2015lumibyls.csv\">2015lumibyls.csv</a> for the <a href=\"/record/14210\">list of validated runs</a> and lumi sections.</p><p>The uncertainty in the luminosity measurement of 2015 data should be considered as 1.6% (reference <a href=\"https://cds.cern.ch/record/2759951\">Precision luminosity measurement in proton-proton collisions at $\\sqrt{s} =$ 13 TeV in 2015 and 2016 at CMS</a>).</p><p>In your estimate for the integrated luminosity, check for which runs the trigger you have selected is active and sum the values for those runs. If you are using prescaled triggers, you can find the trigger prescale factors as shown in <a href=\"https://github.com/cms-opendata-analyses/PhysObjectExtractorTool/blob/2015MiniAOD/PhysObjectExtractor/src/TriggerAnalyzer.cc\">TriggerAnalyzer.cc</a> of the PhysObjectExtractorTool example code. The change of prescales (run, lumi section, index of prescales) is recorded in <a href=\"/record/1055/files/prescale2015.csv\">prescale2015.csv</a></p><p>Additional information on how to extract luminosity values using the <strong>brilcalc tool</strong> can be found in the <a href=\"/docs/cms-guide-luminosity-calculation\"> luminosity calculation guide</a>.</p>"
     },
     "accelerator": "CERN-LHC",
     "collaboration": {