Pixel-by-pixel SBI modeling recovers young massive Pop III clumps at up to 90 percent rate in favorable JWST-like configurations while integrated analyses fail due to contamination.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
NGC 1381 is modeled as having a nuclear disc, BP/X-shaped bar, bulge, thin disc, thick disc and halo, with the bar being ancient and slow and the bulge and thick disc largely accreted.
citing papers explorer
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A Pixel-by-Pixel Path to Population III Discovery with JWST
Pixel-by-pixel SBI modeling recovers young massive Pop III clumps at up to 90 percent rate in favorable JWST-like configurations while integrated analyses fail due to contamination.
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Dissecting the 3D chemo-dynamical structures of NGC 1381: a galaxy hosting an ancient slow bar with an accreted bulge and thick disc
NGC 1381 is modeled as having a nuclear disc, BP/X-shaped bar, bulge, thin disc, thick disc and halo, with the bar being ancient and slow and the bulge and thick disc largely accreted.