A Pan-STARRS1 Search for Planet Nine

Fuente: arXiv
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Main Authors: Brown, Michael E., Holman, Matthew J., Batygin, Konstantin
Format: Preprint
Published: 2024
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author Brown, Michael E.
Holman, Matthew J.
Batygin, Konstantin
author_facet Brown, Michael E.
Holman, Matthew J.
Batygin, Konstantin
contents We present a search for Planet Nine using the second data release of the Pan-STARRS1survey. We rule out the existence of a Planet Nine with the characteristics of that predicted in Brown & Batygin (2021) to a 50% completion depth of $V=21.5$. This survey, along with previous analyses of the Zwicky Transient Facility (ZTF) and Dark EnergySurvey (DES) 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.
format Preprint
id arxiv_https___arxiv_org_abs_2401_17977
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle A Pan-STARRS1 Search for Planet Nine
Brown, Michael E.
Holman, Matthew J.
Batygin, Konstantin
Earth and Planetary Astrophysics
We present a search for Planet Nine using the second data release of the Pan-STARRS1survey. We rule out the existence of a Planet Nine with the characteristics of that predicted in Brown & Batygin (2021) to a 50% completion depth of $V=21.5$. This survey, along with previous analyses of the Zwicky Transient Facility (ZTF) and Dark EnergySurvey (DES) 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.
title A Pan-STARRS1 Search for Planet Nine
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2401.17977