Pith Number
pith:GKGTPEZR
pith:2002:GKGTPEZR7HHNOUDPTDSAYK2LHZ
not attested
not anchored
not stored
refs pending
Cosmic star formation history associated with QSO activity: an approach using the black hole to bulge mass correlation
arxiv:astro-ph/0212534 v1 · 2002-12-24 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GKGTPEZR7HHNOUDPTDSAYK2LHZ}
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 | 2026-07-04T16:31:28.705540Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
328d379331f9ced7506f98e40c2b4b3e52d21969d2603b57a6d4a30b53a3b245
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GKGTPEZR7HHNOUDPTDSAYK2LHZ \
| 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: 328d379331f9ced7506f98e40c2b4b3e52d21969d2603b57a6d4a30b53a3b245
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "bdb93dac0c40da2df109703eca009529e7089258d216418b1e702a8dd51fc18e",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2002-12-24T06:43:32Z",
"title_canon_sha256": "5596cd81ff1ccfed5680548191050c0863748ecb424e0c27fac7cb77271b09c6"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0212534",
"kind": "arxiv",
"version": 1
}
}