pith:AQLEUWVQ
Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies
A transition to low-opacity supernova dust at z>9 reproduces the low UV attenuation and excess of bright galaxies seen by JWST.
arxiv:2605.09829 v2 · 2026-05-11 · astro-ph.GA · astro-ph.CO
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Claims
We find that the observed A_FUV-M_star relation at z > 9 is best reproduced for an intrinsic FUV dust opacity kappa_UV(dust)=1000 cm2/g, characteristic of low-opacity SNe dust, naturally producing very low attenuation even in gas-rich galaxies.
The premise that galaxies at z>9 are dominated by low-opacity SNe-produced dust before efficient ISM grain growth is established, which is invoked to justify the low kappa_UV value and the transition framework.
A transition to low-opacity supernova-produced dust at z>9 reduces effective UV attenuation in gas-rich galaxies and reproduces the observed UV luminosity function and A_FUV-M_star relation.
Formal links
Receipt and verification
| First computed | 2026-05-20T01:06:10.095560Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
04164a5ab076725eb42ed3ce54bfe7dfa578f20e9cd3fbe5db3bd2e0e536be1b
Aliases
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/AQLEUWVQOZZF5NBO2PHFJP7H36 \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 04164a5ab076725eb42ed3ce54bfe7dfa578f20e9cd3fbe5db3bd2e0e536be1b
Canonical record JSON
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