Abstract
We present a search for Planet Nine using the second data release of the Pan-STARRS1 survey. We rule out the existence of a Planet Nine with the characteristics of that predicted in Brown & Batygin to a 50% completion depth of V = 21.5. This survey, along with previous analyses of the Zwicky Transient Facility and Dark Energy Survey data, rules out 78% of the Brown & Batygin parameter space. Much of the remaining parameter space is at V > 21 in regions near and in the area where the northern galactic plane crosses the ecliptic.
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CITATION STYLE
Brown, M. E., Holman, M. J., & Batygin, K. (2024). A Pan-STARRS1 Search for Planet Nine. The Astronomical Journal, 167(4), 146. https://doi.org/10.3847/1538-3881/ad24e9
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