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.
Reumert,et al.,arXiv e-printsp
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JWST absorption spectra of galaxies at z~8-9 show metal-poor gas with high [C/O] suggesting enrichment by Population III supernovae.
A review of theoretical models for the first stars and observational strategies including JWST searches, near-field studies, and lensing, noting growing candidates and narrowing parameter space.
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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Chemical signatures from the first stars embedded in metal-poor gas in galaxies at cosmic dawn
JWST absorption spectra of galaxies at z~8-9 show metal-poor gas with high [C/O] suggesting enrichment by Population III supernovae.
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How can we finally see the first light? Status and perspective in the search for Population III stars
A review of theoretical models for the first stars and observational strategies including JWST searches, near-field studies, and lensing, noting growing candidates and narrowing parameter space.