Pith Number
pith:CCXDISPI
pith:2019:CCXDISPI53KRNHSVBXC54CIEX2
not attested
not anchored
not stored
refs pending
Pulsar Radio Emission Mechanism: Radio Nanoshots as a Low Frequency Afterglow of Relativistic Magnetic Reconnection
arxiv:1902.07730 v1 · 2019-02-20 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{CCXDISPI53KRNHSVBXC54CIEX2}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
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 | 2026-05-17T23:47:25.984881Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
10ae3449e8eed5169e550dc5de0904be9d551f784765ad6cc269350983dd7d40
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CCXDISPI53KRNHSVBXC54CIEX2 \
| 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: 10ae3449e8eed5169e550dc5de0904be9d551f784765ad6cc269350983dd7d40
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "b19528a0ef44aea4961bc5c64cee168ba66feb22a674f304ec38d88f53277008",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2019-02-20T19:02:49Z",
"title_canon_sha256": "bc3469412323a925e28973e7efa00e7ddec80d26cbd18891a40d2b867305c766"
},
"schema_version": "1.0",
"source": {
"id": "1902.07730",
"kind": "arxiv",
"version": 1
}
}