Pith Number
pith:HUO4HGEW
pith:2005:HUO4HGEWEGP4QG5QMF2QDHM2WG
not attested
not anchored
not stored
refs pending
Star Formation Rates in Cooling Flow Clusters: A UV Pilot Study with Archival XMM-Newton Optical Monitor Data
arxiv:astro-ph/0508143 v1 · 2005-08-04 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HUO4HGEWEGP4QG5QMF2QDHM2WG}
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.
Cited by
Receipt and verification
| First computed | 2026-07-04T17:14:58.827081Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3d1dc39896219fc81bb06175019d9ab1878040181c02c307e9c994e8d0382539
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HUO4HGEWEGP4QG5QMF2QDHM2WG \
| 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: 3d1dc39896219fc81bb06175019d9ab1878040181c02c307e9c994e8d0382539
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "684d7f49a045969a1bd16db0559969d1f8f2265e50d5370f119d8560324319a3",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2005-08-04T20:00:03Z",
"title_canon_sha256": "2ffa2125096fd33892c1210cb03f6eb198ad49f9c711d2f1991aa683c4ecc8c8"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0508143",
"kind": "arxiv",
"version": 1
}
}