From 6324f33e0df76419e38575065e8911b0a117cae7 Mon Sep 17 00:00:00 2001
From: galaxyumi <ccamzzichyuk@gmail.com>
Date: Wed, 29 Jul 2026 17:59:43 +0000
Subject: [PATCH] small wording update

---
 .../201_14_IsolatedStarStellarMotions_table.ipynb             | 4 ++--
 1 file changed, 2 insertions(+), 2 deletions(-)

diff --git a/DP2/200_Data_products/201_Catalogs/201_14_IsolatedStarStellarMotions_table.ipynb b/DP2/200_Data_products/201_Catalogs/201_14_IsolatedStarStellarMotions_table.ipynb
index 421466d6..bd02b6ab 100644
--- a/DP2/200_Data_products/201_Catalogs/201_14_IsolatedStarStellarMotions_table.ipynb
+++ b/DP2/200_Data_products/201_Catalogs/201_14_IsolatedStarStellarMotions_table.ipynb
@@ -24,7 +24,7 @@
     "Data Release: <a href=\"https://dp2.lsst.io/\">Data Preview 2</a> <br>\n",
     "Container Size: large <br>\n",
     "LSST Science Pipelines version: r30.0.10 <br>\n",
-    "Last verified to run: 2026-07-22 <br>\n",
+    "Last verified to run: 2026-07-29 <br>\n",
     "Repository: <a href=\"https://github.com/lsst/tutorial-notebooks\">github.com/lsst/tutorial-notebooks</a> <br>"
    ]
   },
@@ -56,7 +56,7 @@
    "source": [
     "## 1. Introduction\n",
     "\n",
-    "The `IsolatedStarStellarMotions` table provides calibrated positions, proper motions, and parallaxes for isolated point sources across the survey footprint. Following single-frame processing, point sources with no nearby neighbors within a $2^{\\prime\\prime}$ radius are identified across all input science images. These isolated sources are cross-matched across multiple overlapping visits and tied to an external reference catalog (Gaia DR3). The global astrometric model is computed jointly across the matched visits using `gbdesAstrometricFitTask`. Each distinct physical star in this catalog is tracked across visits by a unique identifier, `isolated_star_id`.\n",
+    "The `IsolatedStarStellarMotions` table provides calibrated positions, proper motions, and parallaxes for isolated point sources across the survey footprint. Following single-frame processing, point sources with no nearby neighbors within a $2^{\\prime\\prime}$ radius are identified across all input science images. These isolated sources are cross-matched across multiple overlapping visits and tied to an external reference catalog (Gaia DR3). The position, proper motion, and parallax are computed jointly across the matched visits using `FitStellarMotionTask`. Each distinct physical star in this catalog is tracked across visits by a unique identifier, `isolated_star_id`.\n",
     "\n",
     "* TAP table name: `dp2.IsolatedStarStellarMotions`\n",
     "* butler table name: `isolated_star_stellar_motions`\n",