Pith Number
pith:S3HVTLZ6
pith:2024:S3HVTLZ6YHZVU3ZGPQWYTOHBPT
not attested
not anchored
not stored
refs pending
Contribution of the Cygnus bubble to the Galactic cosmic ray spectrum and diffuse $\gamma$-ray emissions
arxiv:2408.01693 v1 · 2024-08-03 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{S3HVTLZ6YHZVU3ZGPQWYTOHBPT}
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 | 2026-07-05T08:52:01.365432Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
96cf59af3ec1f35a6f267c2d89b8e17cf860a01b430e5ae2c534cdc47c109f65
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/S3HVTLZ6YHZVU3ZGPQWYTOHBPT \
| 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: 96cf59af3ec1f35a6f267c2d89b8e17cf860a01b430e5ae2c534cdc47c109f65
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d25efcc8cf9894242b576be7459a393ad36b914b2babafe81f2ccfeb459b42ad",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2024-08-03T07:24:29Z",
"title_canon_sha256": "54d49cc8781efd4785d066025bc99216779303c6894321e96927100f706b27f0"
},
"schema_version": "1.0",
"source": {
"id": "2408.01693",
"kind": "arxiv",
"version": 1
}
}