Merge pull request #42 from lsst/u/rlau/diasource_reliability

Reliability score edits from Fed and Tatiana. Bypassed mobu checks (MLG) b/c not changes to code.

Author: MelissaGraham

DP1/200_Data_Products/201_Catalogs/201_5_DiaSource_table.ipynb

@@ -36,7 +36,7 @@
     "\n",
     "**Packages:** `lsst.rsp`, `lsst.daf.butler`\n",
     "\n",
-    "**Credit:** Originally developed by the Rubin Community Science team with feedback from Eric Bellm.\n",
+    "**Credit:** Originally developed by the Rubin Community Science team with feedback from Eric Bellm, Federica Bianco, and Tatiana Cuellar.\n",
     "Please consider acknowledging them if this notebook is used for the preparation of journal articles, software releases, or other notebooks.\n",
     "\n",
     "**Get Support:**\n",
@@ -417,7 +417,7 @@
     "\n",
     "* `reliability`\n",
     "\n",
-    "The purpose of the `reliability` score in the `DiaSource` table is to provide a threshold measure to improve the purity of transient detections. This score is computed using information from the source and image characterization, as well as the information on the Telescope and Camera system. However, given that the reliability score model was trained on a relatively small and limited dataset, some caution is warranted in interpreting the `reliability` score in DP1, in particular for variable stars. Significant improvements are expected on future releases with LSSTCam data."
+    "The purpose of the `reliability` score in the `DiaSource` table is to provide a threshold measure to improve the purity of DIA detections. This score is computed using information from the source and image characterization, as well as the information on the Telescope and Camera system. However, given that the reliability score model was trained on a relatively small and limited dataset, some caution is warranted in interpreting the `reliability` score in DP1, in particular for variable stars. Significant improvements are expected on future releases with LSSTCam data."
    ]
   },
   {