Pith Number
pith:YAQEM6XB
pith:2005:YAQEM6XBW2V5HWMTCP3DSBIWFU
not attested
not anchored
not stored
refs pending
Ultraviolet Dust Grain Properties in Starburst Galaxies: Evidence from Radiative Transfer Modeling and Local Group Extinction Curves
arxiv:astro-ph/0501413 v2 · 2005-01-19 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YAQEM6XBW2V5HWMTCP3DSBIWFU}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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claim
4
Citations
5
Replications
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Portable graph bundle live · download bundle · merged
state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Receipt and verification
| First computed | 2026-07-04T16:50:40.176399Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c020467ae1b6abd3d99313f63905162d3064bf40b6c66342ae1474b4d5788c89
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YAQEM6XBW2V5HWMTCP3DSBIWFU \
| 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: c020467ae1b6abd3d99313f63905162d3064bf40b6c66342ae1474b4d5788c89
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3d72c628d2099642cc1361ed0d43aea4e1afc9dbede3c1f44c634c05c9ec661a",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2005-01-19T15:47:47Z",
"title_canon_sha256": "d7daa9a2549778d2c9edff4f9a1d12c2023207c3b88aa4d656ef147268d53b05"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0501413",
"kind": "arxiv",
"version": 2
}
}