Pith Number
pith:B3Q4F2ME
pith:2010:B3Q4F2ME4XSSCQTQP7TGRQQFY4
not attested
not anchored
not stored
refs pending
Quantifying Kinematic Substructure in the Milky Way's Stellar Halo
arxiv:1011.1925 v2 · 2010-11-08 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{B3Q4F2ME4XSSCQTQP7TGRQQFY4}
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 | 2026-05-18T04:15:28.386608Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0ee1c2e984e5e52142707fe668c205c72e261d83ac2f172b1a69d92c7d38d313
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/B3Q4F2ME4XSSCQTQP7TGRQQFY4 \
| 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: 0ee1c2e984e5e52142707fe668c205c72e261d83ac2f172b1a69d92c7d38d313
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "993e4bbc8b806197fe1d154feaa14323c23afcc66afdd0fe4987d932b777bde9",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2010-11-08T21:38:04Z",
"title_canon_sha256": "991e49ded37b9be064e49902d398e6590cb9febf5772bdc50bca212559cbb932"
},
"schema_version": "1.0",
"source": {
"id": "1011.1925",
"kind": "arxiv",
"version": 2
}
}