Pith Number
pith:YXX7QJBE
pith:2008:YXX7QJBEQLAFRVA3KJBRPYXFT5
not attested
not anchored
not stored
refs pending
Physical conditions in potential sources of ultra-high-energy cosmic rays: Updated Hillas plot and radiation-loss constraints
arxiv:0808.0367 v2 · 2008-08-04 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YXX7QJBEQLAFRVA3KJBRPYXFT5}
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 | 2026-05-18T02:35:15.417771Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c5eff8242482c058d41b524317e2e59f4ce6023dbfe43c352123ac47f6c7c2a5
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YXX7QJBEQLAFRVA3KJBRPYXFT5 \
| 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: c5eff8242482c058d41b524317e2e59f4ce6023dbfe43c352123ac47f6c7c2a5
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "31f0539847d1a99caff916a8ba2cc823c5275cccbc1183cca18b66782a29229a",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph",
"submitted_at": "2008-08-04T18:27:49Z",
"title_canon_sha256": "89a445b91f99aefe67c9e2769088ca6a2f97301dc144c81c1e99ef5703490f4b"
},
"schema_version": "1.0",
"source": {
"id": "0808.0367",
"kind": "arxiv",
"version": 2
}
}