pith:4H6CYHVC
High-fidelity stellar extinction with Gaia and APOGEE -- I. The method and a new extinction curve
Stellar extinction for APOGEE stars is measured to 0.03 mag precision by training an XGBoost model on minimally reddened stars and anchoring to a Gaia BP/RP ratio of 1.694.
arxiv:2601.10595 v2 · 2026-01-15 · astro-ph.SR · astro-ph.GA
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Claims
Our extinction estimates (Av) outperform existing results (Bayestar19, StarHorse, SEDEX), achieving a typical precision of 0.03 mag in Av. Notably, we identify systematic deviations of up to 30% between monochromatic and passband-integrated extinction ratios at wavelengths greater than 700 nm.
The assumption that a training set of minimally reddened stars exists and can be reliably identified to train the XGBoost model for intrinsic colors without residual dust bias.
Machine learning derives 0.03 mag precision Av extinctions for APOGEE stars and a new passband-specific extinction curve showing up to 30% deviations from monochromatic ratios beyond 700 nm.
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| First computed | 2026-05-17T23:39:16.651016Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e1fc2c1ea203081a78d5b5dd3aa02b01422da4d7ec1660055196171b34c7eb9f
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/4H6CYHVCAMEBU6GVWXOTVIBLAF \
| 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: e1fc2c1ea203081a78d5b5dd3aa02b01422da4d7ec1660055196171b34c7eb9f
Canonical record JSON
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