Pith Number
pith:QYPWYYPY
pith:2001:QYPWYYPYHFRFBHEGWTCBW7JQHD
not attested
not anchored
not stored
refs pending
Dynamical evolution of clusters of galaxies: the effect of high- velocity substructure clumps
arxiv:astro-ph/0112561 v2 · 2001-12-29 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{QYPWYYPYHFRFBHEGWTCBW7JQHD}
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 | 2026-05-18T01:09:10.810964Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
861f6c61f83962509c86b4c41b7d3038f4c4313c8a0309ed5ac49bc1ccf25b65
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/QYPWYYPYHFRFBHEGWTCBW7JQHD \
| 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: 861f6c61f83962509c86b4c41b7d3038f4c4313c8a0309ed5ac49bc1ccf25b65
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3fb27158b823516d4629ff050aba8bfa96fd80b19a3544ad2fb38db8ab06d114",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2001-12-29T16:11:34Z",
"title_canon_sha256": "4474d06e57fe7f8d1f2326a89d5e209d0366bd90714da8b3eea6b574a24a5344"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0112561",
"kind": "arxiv",
"version": 2
}
}