Pith Number
pith:CZOQ5KE6
pith:2019:CZOQ5KE6QS2L55SBUUNNRORCGU
not attested
not anchored
not stored
refs pending
Frequency drifts in FRBs due to radius-to-frequency mapping in magnetospheres of neutron stars
arxiv:1908.07313 v1 · 2019-08-19 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{CZOQ5KE6QS2L55SBUUNNRORCGU}
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 | 2026-07-04T23:58:33.073301Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
165d0ea89e84b4bef641a51ad8ba2235186fd3df2ad6aef5ed857031f1caa2b2
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CZOQ5KE6QS2L55SBUUNNRORCGU \
| 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: 165d0ea89e84b4bef641a51ad8ba2235186fd3df2ad6aef5ed857031f1caa2b2
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "da80931c2a16d99ac85dd378e0f24fbbe62cd37418261c3aa8efaf54d2feb728",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2019-08-19T17:45:30Z",
"title_canon_sha256": "5e78e11f757331348b3c5464e0ac334f51e7bd83e8f3fa96362305e144bbcee0"
},
"schema_version": "1.0",
"source": {
"id": "1908.07313",
"kind": "arxiv",
"version": 1
}
}