Pith Number
pith:Q5YHGIW2
pith:2001:Q5YHGIW26K2KDWI7BSH7QAH5MK
not attested
not anchored
not stored
refs pending
The X-ray surface brightness profiles of hot galaxy clusters up to z~0.8: evidence for self-similarity and constraints on Omega_0
arxiv:astro-ph/0110428 v2 · 2001-10-18 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{Q5YHGIW26K2KDWI7BSH7QAH5MK}
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 | 2026-07-04T16:24:18.809210Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
87707322daf2b4a1d91f0c8ff800fd62abbdfc72504b3d5baf5db3620e84b44b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Q5YHGIW26K2KDWI7BSH7QAH5MK \
| 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: 87707322daf2b4a1d91f0c8ff800fd62abbdfc72504b3d5baf5db3620e84b44b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "12ab2a797310950f82bd55a196260d29534bf5bcc5182291e42160132ae32f8c",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2001-10-18T18:32:56Z",
"title_canon_sha256": "bab2ca81672a7668993580869420e1b0004c007e1586f114c22b70744daa6473"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0110428",
"kind": "arxiv",
"version": 2
}
}