Pith Number
pith:3F25KLLL
pith:2018:3F25KLLLTITEA7JQL3MXVPSSWX
not attested
not anchored
not stored
refs pending
Synchrotron maser from weakly magnetised neutron stars as the emission mechanism of fast radio bursts
arxiv:1806.02700 v2 · 2018-06-07 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3F25KLLLTITEA7JQL3MXVPSSWX}
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.
Cited by
Receipt and verification
| First computed | 2026-05-17T23:49:43.699559Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d975d52d6b9a26407d305ed97abe52b5ecb831084626a494a616945818b2b568
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3F25KLLLTITEA7JQL3MXVPSSWX \
| 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: d975d52d6b9a26407d305ed97abe52b5ecb831084626a494a616945818b2b568
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dee0452c463e5e6b332f405add90ca3dee646aaf2e1bce92d5c549eb4e35ab67",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-06-07T14:26:53Z",
"title_canon_sha256": "63d618a97efeaf0873807b9fd556d78e4a67dedd6006fe548635a26c838249f8"
},
"schema_version": "1.0",
"source": {
"id": "1806.02700",
"kind": "arxiv",
"version": 2
}
}