Pith Number
pith:VGNBHV7U
pith:2014:VGNBHV7USFPE4BDIYVAECJ3FHX
not attested
not anchored
not stored
refs pending
Using the morphology and magnetic fields of tailed radio galaxies as environmental probes
arxiv:1412.8596 v1 · 2014-12-30 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{VGNBHV7USFPE4BDIYVAECJ3FHX}
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 | 2026-05-18T01:41:15.235939Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a99a13d7f4915e4e0468c5404127653dfeaa150508b7f4408f5287584158ec1b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/VGNBHV7USFPE4BDIYVAECJ3FHX \
| 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: a99a13d7f4915e4e0468c5404127653dfeaa150508b7f4408f5287584158ec1b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "73a68db1a1d3e8eb7679701248c830757a52189fdeb1b894b7e5937052d770b8",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-12-30T10:16:07Z",
"title_canon_sha256": "da65544aa70d7ed163decce5c22f8095f418d829ef3b54d00582336579a4b673"
},
"schema_version": "1.0",
"source": {
"id": "1412.8596",
"kind": "arxiv",
"version": 1
}
}