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Foreman-Mackey, D · 2013

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fields

astro-ph.EP 1 astro-ph.HE 1

years

2026 2

verdicts

CONDITIONAL 1 UNVERDICTED 1

representative citing papers

The pair-instability origin of supernova 2023vbw

astro-ph.HE · 2026-05-15 · conditional · novelty 6.0

Observations and modeling of SN 2023vbw indicate it is a pair-instability supernova with ejecta mass 170-350 solar masses, nickel mass 1.2-1.6 solar masses, and explosion energy (6-13) x 10^52 erg.

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Showing 2 of 2 citing papers.

  • Aerosols and hydrocarbons in the atmosphere of a white dwarf planet astro-ph.EP · 2026-07-01 · unverdicted · none · ref 8

    JWST NIRSpec PRISM transmission spectroscopy detects CH4, other hydrocarbons, and aerosols in WD 1856 b's atmosphere, with evidence for recent reheating and a carbon-enriched composition.

  • The pair-instability origin of supernova 2023vbw astro-ph.HE · 2026-05-15 · conditional · none · ref 58

    Observations and modeling of SN 2023vbw indicate it is a pair-instability supernova with ejecta mass 170-350 solar masses, nickel mass 1.2-1.6 solar masses, and explosion energy (6-13) x 10^52 erg.