Pith Number
pith:4BTW3C7V
pith:2004:4BTW3C7VNISZR5JPNTRPLDG5IF
not attested
not anchored
not stored
refs pending
Of NBOs and kHz QPOs: a low-frequency modulation in resonant oscillations of relativistic accretion disks
arxiv:astro-ph/0408090 v1 · 2004-08-04 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4BTW3C7VNISZR5JPNTRPLDG5IF}
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 | 2026-05-18T01:40:35.172014Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e0676d8bf56a2598f52f6ce2f58cdd417aad861788d04a8d48e61206c9100b2c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4BTW3C7VNISZR5JPNTRPLDG5IF \
| 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: e0676d8bf56a2598f52f6ce2f58cdd417aad861788d04a8d48e61206c9100b2c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "be671c9906b71eef20f72b682d5b4ceebe74015b6b5df5fcce5df6e3343af85f",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2004-08-04T17:30:10Z",
"title_canon_sha256": "2e5207498e6e8a4f4831b1ab6b70f240ea4c90df9538910d33dab2dac74f55a3"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0408090",
"kind": "arxiv",
"version": 1
}
}