pith:IOGO5ADW
A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS
New 3D dust map uses Gaia parallaxes and a spatial prior for smoother clouds with smaller uncertainties.
arxiv:1905.02734 v1 · 2019-05-07 · astro-ph.GA
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Claims
This new map contains three major improvements over our previous work: inclusion of Gaia parallaxes for better distances, a spatial prior correlating dust density across nearby sightlines, and four times finer distance resolution.
The spatial prior that correlates dust density across nearby sightlines will produce a smoother map with more isotropic clouds and smaller distance uncertainties, particularly within the nearest kiloparsec.
A new 3D dust reddening map with finer distance resolution, a spatial correlation prior, and Gaia-based distances covering the sky north of -30 degrees declination out to several kiloparsecs.
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| First computed | 2026-05-17T23:38:50.307619Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/IOGO5ADWIK466J5EJ6GLSUKYSO \
| 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())"
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Canonical record JSON
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