Pith Number
pith:M3VKCHLM
pith:2012:M3VKCHLMAVFVYFF4YHPY34RV7F
not attested
not anchored
not stored
refs pending
Updated Mass Scaling Relations for Nuclear Star Clusters and a Comparison to Supermassive Black Holes
arxiv:1205.5338 v2 · 2012-05-24 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{M3VKCHLMAVFVYFF4YHPY34RV7F}
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 | 2026-05-18T03:34:14.100962Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
66eaa11d6c054b5c14bcc1df8df235f975fbf597bcc758edf3594c33db81fb90
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/M3VKCHLMAVFVYFF4YHPY34RV7F \
| 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: 66eaa11d6c054b5c14bcc1df8df235f975fbf597bcc758edf3594c33db81fb90
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d053aca9c1fa95e8af5cd2ff02a0bafd96828e7d4169cc42f0d2701243aa575e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2012-05-24T06:11:03Z",
"title_canon_sha256": "ef809b5e30f2a9324ad62cea829886f4aa8f454e9a1ba3d15a90468930e8700c"
},
"schema_version": "1.0",
"source": {
"id": "1205.5338",
"kind": "arxiv",
"version": 2
}
}