Pith Number
pith:XPVVZZ4A
pith:2014:XPVVZZ4AFZYR5GBZ7UOOHQXD4W
not attested
not anchored
not stored
refs pending
The relation between radio and X-ray luminosity of black hole binaries: affected by inner cool disks?
arxiv:1401.7525 v1 · 2014-01-29 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XPVVZZ4AFZYR5GBZ7UOOHQXD4W}
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 | 2026-05-18T01:44:55.074537Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
bbeb5ce7802e711e9839fd1ce3c2e3e5950d013730826d5b692ee6c1ce5a7cd9
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XPVVZZ4AFZYR5GBZ7UOOHQXD4W \
| 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: bbeb5ce7802e711e9839fd1ce3c2e3e5950d013730826d5b692ee6c1ce5a7cd9
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2a3a07333ca33d36a4bcab0fd0efb3f1b51fdfc4ec87cc55b165704097969fe6",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2014-01-29T14:43:36Z",
"title_canon_sha256": "d3bde267c901f833751306f279d49fce25183cd6dd1ca29f4d84ccdb26b1d4c9"
},
"schema_version": "1.0",
"source": {
"id": "1401.7525",
"kind": "arxiv",
"version": 1
}
}