Pith Number
pith:KQQPLJ6J
pith:2011:KQQPLJ6JZLLVBAFR5DM4IP5Y5E
not attested
not anchored
not stored
refs pending
The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos
arxiv:1104.5040 v1 · 2011-04-26 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KQQPLJ6JZLLVBAFR5DM4IP5Y5E}
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 | 2026-05-18T02:02:14.454834Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5420f5a7c9cad75080b1e8d9c43fb8e925234b0f0b810e207b9b8d1eef548166
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E \
| 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: 5420f5a7c9cad75080b1e8d9c43fb8e925234b0f0b810e207b9b8d1eef548166
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "eb894b5c09b881ca86d9a4e0c6b5a054478172a5b5fbd348d5619b60de008c66",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2011-04-26T22:18:31Z",
"title_canon_sha256": "c687e1731cd356a65cac31dc52c621a28f977e6b481ee1281a992beab32383f7"
},
"schema_version": "1.0",
"source": {
"id": "1104.5040",
"kind": "arxiv",
"version": 1
}
}