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MPC/RFL_Solar_System_MPC_Retrieval.ipynb

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"\n",
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"</div>\n",
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"\n",
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"For the Rubin Science Platform at data.lsst.cloud. <br>\n",
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"For Solar System object discoveries released as part of Rubin First Look. <br>\n",
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"Container Size: large <br>\n",
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"LSST Science Pipelines version: r29.2.0 <br>\n",
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"Last verified to run: 2025-09-02 <br>\n",
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"Repository: <a href=\"https://github.com/lsst/tutorial-notebooks\">github.com/lsst/tutorial-notebooks</a> <br>\n"
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"For the Rubin Science Platform at data.lsst.cloud.\\\n",
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"For Solar System object discoveries released as part of Rubin First Look.\\\n",
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"Container Size: large\\\n",
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"LSST Science Pipelines version: r29.2.0\\\n",
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"Last verified to run: 2025-11-25\\\n",
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"Repository: [github.com/lsst/tutorial-notebooks](https://github.com/lsst/tutorial-notebooks)\\\n",
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"DOI: [10.11578/rubin/dc.20250909.20](https://doi.org/10.11578/rubin/dc.20250909.20)"
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"\n",
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"**LSST data products:** Small body observations made by Rubin, queried from the Minor Planet Center (MPC), and orbits computed by the MPC from those Rubin observations are used in the notebook. No direct LSST data products are used in this notebook.\n",
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"\n",
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"**Packages:** `get_orb` and `get_obs` <a href=\"https://www.minorplanetcenter.net/mpcops/documentation/\">APIs from the Minor Planet Center</a>.\n",
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"**Packages:** `get_orb` and `get_obs` [APIs from the Minor Planet Center](https://www.minorplanetcenter.net/mpcops/documentation/).\n",
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"\n",
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"**Credit:**\n",
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"Originally developed by Sarah Greenstreet and Mario Juric from the Rubin Community Science team, Solar System Processing (SSP) team and Solar System Commissioning science unit. Please consider acknowledging them if this notebook is used for the preparation of journal articles, software releases, or other notebooks.\n",
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"\n",
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"**Get Support:**\n",
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"Everyone is encouraged to ask questions or raise issues in the <a href=\"https://community.lsst.org/c/support\">Support Category</a> \n",
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"of the Rubin Community Forum. Rubin staff will respond to all questions posted there."
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"Everyone is encouraged to ask questions or raise issues in the [Support Category](https://community.lsst.org/c/support) of the Rubin Community Forum.\n",
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"Rubin staff will respond to all questions posted there."
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"source": [
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"### 1.1. Import packages\n",
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"\n",
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"Import `numpy`, a fundamental package for scientific computing with arrays in Python\n",
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"(<a href=\"https://numpy.org\">numpy.org</a>), and\n",
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"`matplotlib`, a comprehensive library for data visualization\n",
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"(<a href=\"https://matplotlib.org/\">matplotlib.org</a>; \n",
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"<a href=\"https://matplotlib.org/stable/gallery/index.html\">matplotlib gallery</a>)."
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"Import `numpy`, a fundamental package for scientific computing with arrays in Python ([numpy.org](https://numpy.org)), and\n",
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"`matplotlib`, a comprehensive library for data visualization ([matplotlib.org](https://matplotlib.org/); [matplotlib gallery](https://matplotlib.org/stable/gallery/index.html))."
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"id": "a928a607-9977-4a09-b689-9efeb49b8437",
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"metadata": {},
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"source": [
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"Plot the semimajor axes, eccentricities, and inclinations of the 2,098 Rubin First Look Solar System object discoveries. Use the orbit types defined by the MPC (https://minorplanetcenter.net/mpcops/documentation/orbit-types/) to distinguish each orbital classification in the plot.\n"
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"Plot the semimajor axes, eccentricities, and inclinations of the 2,098 Rubin First Look Solar System object discoveries.\n",
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"Use the [orbit types defined by the MPC](https://minorplanetcenter.net/mpcops/documentation/orbit-types/) to distinguish each orbital classification in the plot."
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"id": "4a447a05-0d3a-435a-a28a-2b1f45865444",
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"metadata": {},
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"source": [
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"> **Figure 3:** The log of the number of photometric measurements with a given `rmsmag` value. The grey line is drawn at $0.25$ mag, the approximate (by-eye) division between the distribution of `rmsmag` values and the tail of \"outliers\"."
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"> **Figure 3:** The log of the number of photometric measurements with a given `rmsmag` value. The dashed grey line is drawn at $0.25$ mag, the approximate (by-eye) division between the distribution of `rmsmag` values and the tail of \"outliers\"."
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"id": "07571984-17db-4c2d-b297-96d79f088909",
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"metadata": {},
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"The above demonstrates a simple, by-eye evaluation that `rmsmag` $> 0.25` mag indicates an \"outlier\" photometric meaurement for the RFL data sent to the MPC.\n",
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"The above demonstrates a simple, by-eye evaluation that `rmsmag` $> 0.25$ mag indicates an \"outlier\" photometric meaurement for the RFL data sent to the MPC.\n",
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"\n",
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"Inclusion of these data points in any analysis should be done with caution."
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