Pith Number
pith:ISQTN6RR
pith:1994:ISQTN6RREMYIKAZQ4XEI2AXD6V
not attested
not anchored
not stored
refs pending
Light Element Abundance Inhomogeneities in Globular Clusters: Probing Star Formation and Evolution in the Early Milky Way
arxiv:astro-ph/9408007 v1 · 1994-08-02 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{ISQTN6RREMYIKAZQ4XEI2AXD6V}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T01:40:24.460976Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
44a136fa312330850330e5c88d02e3f5748ed1dbcdb153cfdc77aa1b75b8f7e8
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/ISQTN6RREMYIKAZQ4XEI2AXD6V \
| 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: 44a136fa312330850330e5c88d02e3f5748ed1dbcdb153cfdc77aa1b75b8f7e8
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "11717b16da6e6caad1e401a30797cc2e5cb31d324874f342d86f2e4269c88ebe",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1994-08-02T19:02:44Z",
"title_canon_sha256": "6556e643da7375510c04c7542841b89333394e03a6c2fc6fb2db039756c86dc6"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9408007",
"kind": "arxiv",
"version": 1
}
}