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"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>"
]
},
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"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",
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