Pith Number
pith:RXEH66F2
pith:2009:RXEH66F2GJPWBSCYTIPVEKT6DE
not attested
not anchored
not stored
refs pending
Formation of an O-Star Cluster by Hierarchical Accretion in G20.08-0.14 N
arxiv:0910.2270 v2 · 2009-10-12 · astro-ph.GA · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RXEH66F2GJPWBSCYTIPVEKT6DE}
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 | 2026-05-18T02:11:24.340760Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8dc87f78ba325f60c8589a1f522a7e1925d8566a54e159b3a18f977b994ed19f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RXEH66F2GJPWBSCYTIPVEKT6DE \
| 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: 8dc87f78ba325f60c8589a1f522a7e1925d8566a54e159b3a18f977b994ed19f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5d2812db37cb7afc3b68c6a901c5bf2aa233b8dde9bb031ef66afa82fd504891",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2009-10-12T23:33:44Z",
"title_canon_sha256": "4e5a09e45c8e4e9db61d91dff1e76678d058f9d17d58a366453abd896e7c06ab"
},
"schema_version": "1.0",
"source": {
"id": "0910.2270",
"kind": "arxiv",
"version": 2
}
}