A Pan-STARRS1 Search for Planet Nine

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 Tra...
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Gespeichert in:

Autor*in:	Michael E. Brown [verfasserIn] Matthew J. Holman [verfasserIn] Konstantin Batygin [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2024

Schlagwörter:	Sky surveys Solar system gas giant planets

Übergeordnetes Werk:	In: The Astronomical Journal - IOP Publishing, 2022, 167(2024), 4, p 146
Übergeordnetes Werk:	volume:167 ; year:2024 ; number:4, p 146

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-3881/ad24e9

Katalog-ID:	DOAJ097138320

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source	In The Astronomical Journal 167(2024), 4, p 146 volume:167 year:2024 number:4, p 146
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callnumber-first	Q - Science
author	Michael E. Brown
spellingShingle	Michael E. Brown misc QB1-991 misc Sky surveys misc Solar system gas giant planets misc Astronomy A Pan-STARRS1 Search for Planet Nine
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topic_title	QB1-991 A Pan-STARRS1 Search for Planet Nine Sky surveys Solar system gas giant planets
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title	A Pan-STARRS1 Search for Planet Nine
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title_full	A Pan-STARRS1 Search for Planet Nine
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title_sort	pan-starrs1 search for planet nine
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title_auth	A Pan-STARRS1 Search for Planet Nine
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.
abstractGer	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.
abstract_unstemmed	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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container_issue	4, p 146
title_short	A Pan-STARRS1 Search for Planet Nine
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