pith:OQSZEZHU
TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars
Surface brightness of lensed host arcs sets the precision of mass models in doubly imaged quasars.
arxiv:2604.24908 v2 · 2026-04-27 · astro-ph.CO · astro-ph.GA
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Claims
We find a strong correlation between Fermat potential precision and the surface brightness of the spatially extended host arcs, establishing that arc surface brightness is the primary driver of mass model precision in doubly imaged systems.
The tailored Lenstronomy pipeline for doubles accurately captures the lensing geometry and mass profiles without significant biases from data heterogeneity or unaccounted systematics.
Uniform modeling of eight double quasar lenses shows that host arc surface brightness determines Fermat potential precision.
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| First computed | 2026-08-07T00:51:35.090928Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
74259264f4e27fb9fe65ebb4eff4a4258c98056618344a783a5966016a8a3ad8
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/OQSZEZHU4J73T7TF5O2O75FEEW \
| 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: 74259264f4e27fb9fe65ebb4eff4a4258c98056618344a783a5966016a8a3ad8
Canonical record JSON
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