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Python Jupyter notebook shows an example, including all the necessary code.
The tools provided to search for Pan-STARRS1 catalog and to extract images rely on the target positions on the sky. For solar system targets, the position changes with time. This page describes an effective approach for using the known orbits of solar system targets to search both the images and catalogs for PS1 measurements. ATable of Contents | ||
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Overview
174361 Rickwhite (2002 TV315). The Canadian Astronomy Data Centre (CADC) solar system image search API is used to get an initial list of PS1 observations. Then the JPL Horizons database is queried (using the astroquery.jplhorizons
module) to get the position of the target as seen from the PS1 observatory on Mt Haleakala at the exact times of the PS1 observations. Those positions are passed to the PS1 CasJobs database where they are cross-matched with the PS1 detection catalog.
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