Pith Number
pith:OPFW6CNZ
pith:2011:OPFW6CNZ6BZ3DQGDP2ISEFKNXH
not attested
not anchored
not stored
refs pending
Do Nuclear Star Clusters and Black Holes Follow the Same Host-Galaxy Correlations?
arxiv:1112.2740 v1 · 2011-12-12 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OPFW6CNZ6BZ3DQGDP2ISEFKNXH}
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 | 2026-05-18T03:38:05.083590Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
73cb6f09b9f073b1c0c37e9122154db9d55729c84acfa944e3b6855d95e6584a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OPFW6CNZ6BZ3DQGDP2ISEFKNXH \
| 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: 73cb6f09b9f073b1c0c37e9122154db9d55729c84acfa944e3b6855d95e6584a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "bdeaa20b2470ff84dffcebe8c7d3f274abe273e36db7eb7864bab10ef03b3120",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2011-12-12T22:58:02Z",
"title_canon_sha256": "db4a17415a5fd58332bc7de9a217f7741817bb8589e7cf311d861c29377d9e4d"
},
"schema_version": "1.0",
"source": {
"id": "1112.2740",
"kind": "arxiv",
"version": 1
}
}