Pith Number
pith:KWX5YWG6
pith:2009:KWX5YWG6QSYPCP2V7Y6GFOXJBA
not attested
not anchored
not stored
refs pending
The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys
arxiv:0904.3248 v2 · 2009-04-21 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KWX5YWG6QSYPCP2V7Y6GFOXJBA}
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 | 2026-05-18T04:37:34.227915Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
55afdc58de84b0f13f55fe3c62bae9081df4daae669cf7c1b063463c9ed6adcb
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KWX5YWG6QSYPCP2V7Y6GFOXJBA \
| 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: 55afdc58de84b0f13f55fe3c62bae9081df4daae669cf7c1b063463c9ed6adcb
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "9994bd9b04737e0465f39c6e4305e2f3531d6c58620cd82162c41808fd49708b",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2009-04-21T13:20:27Z",
"title_canon_sha256": "bcaf51d20af3c7c1589f8192056b388f12097c80748800be1057ed1c441956e1"
},
"schema_version": "1.0",
"source": {
"id": "0904.3248",
"kind": "arxiv",
"version": 2
}
}