Pith Number
pith:436KEBMC
pith:2011:436KEBMC2GBLFQXOM6UYYS7R2C
not attested
not anchored
not stored
refs pending
On the pulse--width statistics in radio pulsars. I. Importance of the interpulse emission
arxiv:1102.3348 v1 · 2011-02-16 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{436KEBMC2GBLFQXOM6UYYS7R2C}
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 | 2026-05-18T04:19:13.208563Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e6fca20582d182b2c2ee67a98c4bf1d0b47c0eedc4b636d355ad51414f43be1d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/436KEBMC2GBLFQXOM6UYYS7R2C \
| 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: e6fca20582d182b2c2ee67a98c4bf1d0b47c0eedc4b636d355ad51414f43be1d
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dfecf0786722ca0d9373bbc15948e1f27c4d7eabee02fcf2c296871b1696730a",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2011-02-16T14:39:40Z",
"title_canon_sha256": "b9283e0df110046249f6da5752f7a5f3b3b84d1798fd6f7f9a7197db3d3e9175"
},
"schema_version": "1.0",
"source": {
"id": "1102.3348",
"kind": "arxiv",
"version": 1
}
}