Pith Number
pith:UGLQIIYI
pith:2011:UGLQIIYIADX62PFBEXNGBETVVH
not attested
not anchored
not stored
refs pending
Star Clusters in M 31. IV. A Comparative Analysis of Absorption Line Indices in Old M 31 and Milky Way Clusters
arxiv:1112.2737 v1 · 2011-12-12 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{UGLQIIYIADX62PFBEXNGBETVVH}
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
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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 | 2026-05-18T01:59:11.274121Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a19704230800efed3ca125da609275a9c24e952914620e9fa5b19d7171414103
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UGLQIIYIADX62PFBEXNGBETVVH \
| 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: a19704230800efed3ca125da609275a9c24e952914620e9fa5b19d7171414103
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "6425fcb443ad438ddaedff7d455adc2158277371ec526f64cad6fb77a587460a",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2011-12-12T22:28:34Z",
"title_canon_sha256": "3ebd230038557eeb77f8d0c464f17efe9ac8f5a5173b39afff95a41fc857ecd2"
},
"schema_version": "1.0",
"source": {
"id": "1112.2737",
"kind": "arxiv",
"version": 1
}
}