A Pan-STARRS Search For Distant Planets: Part 1

We present a search for distant planets in Pan-STARRS1. We calibrated our search by injecting an isotropic control population of synthetic detections into Pan-STARRS1 source catalogs, providing a high-fidelity alternative to injecting synthetic sources at the image level.
We found that our method is sensitive to a wide range of distances, as well as all rates and directions of motion. We identified 692 solar system objects (109 of which are not yet listed in the Minor Planet Center’s database), including 642 TNOs, 23 of which are dwarf planets.
By raw number of detections, this makes our search the third most productive Kuiper Belt survey to date, in spite of the fact that we did not explicitly search for objects closer than 80 au.
Although we did not find Planet Nine or any other planetary objects, we were able to show that the remaining parameter space for Planet Nine is highly concentrated in the galactic plane.
Matthew J. Holman, Kevin J. Napier, Matthew J. Payne, Jacob A. Kurlander
Comments: 23 pages, 9 figures. PSJ accepted 2025 May 23
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2506.02144 [astro-ph.EP] (or arXiv:2506.02144v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2506.02144
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Submission history
From: Matthew J. Holman
[v1] Mon, 2 Jun 2025 18:13:46 UTC (11,019 KB)
https://arxiv.org/abs/2506.02144
Astrobiology,