Pith Number
pith:GNK2MBQK
pith:2012:GNK2MBQKQAJZX2F2JGEYUA2F3A
not attested
not anchored
not stored
refs pending
Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk
arxiv:1201.1635 v1 · 2012-01-08 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GNK2MBQKQAJZX2F2JGEYUA2F3A}
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 | 2026-05-18T01:58:54.393667Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3355a6060a80139be8ba49898a0345d823dd256ff3b7ab67f2a02c8dcaede921
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GNK2MBQKQAJZX2F2JGEYUA2F3A \
| 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: 3355a6060a80139be8ba49898a0345d823dd256ff3b7ab67f2a02c8dcaede921
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cf5bf116165ca11acb2d675fbbdbdfa0084117a23685a1e926618774d88f514f",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2012-01-08T15:25:20Z",
"title_canon_sha256": "55286fee753102a544f6952381ee7696a6a771a258eafa4f1bbbe4b308f1b154"
},
"schema_version": "1.0",
"source": {
"id": "1201.1635",
"kind": "arxiv",
"version": 1
}
}