Pith Number
pith:IID6AGMN
pith:2011:IID6AGMNWYWE5GLFMBZMUHJ34K
not attested
not anchored
not stored
refs pending
The low frequency of dual AGNs versus the high merger rate of galaxies: A phenomenological model
arxiv:1105.1963 v1 · 2011-05-10 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IID6AGMNWYWE5GLFMBZMUHJ34K}
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 | 2026-05-18T02:02:01.911200Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4207e0198db62c4e99656072ca1d3be28f1aaa8ab1d07c8159aba993e081c050
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IID6AGMNWYWE5GLFMBZMUHJ34K \
| 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: 4207e0198db62c4e99656072ca1d3be28f1aaa8ab1d07c8159aba993e081c050
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "33a9bc5a96e79883b0c13a2a6ed31ec0dff534c36a640730731f68e87a8fe11b",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2011-05-10T14:44:38Z",
"title_canon_sha256": "0a9d9adba765693998331c3fa252d222a946977141bdae6d17c27e15fac10a3c"
},
"schema_version": "1.0",
"source": {
"id": "1105.1963",
"kind": "arxiv",
"version": 1
}
}