Pith Number
pith:2VOZKBLB
pith:2022:2VOZKBLB4QWCV674WLZNEVH26R
not attested
not anchored
not stored
refs pending
What sources are the dominant Galactic cosmic-ray accelerators?
arxiv:2212.10677 v2 · 2022-12-20 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{2VOZKBLB4QWCV674WLZNEVH26R}
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 | 2026-07-05T05:28:10.518361Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d55d950561e42c2afbfcb2f2d254faf4625a024c9f959c74785c62f48acd36e7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2VOZKBLB4QWCV674WLZNEVH26R \
| 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: d55d950561e42c2afbfcb2f2d254faf4625a024c9f959c74785c62f48acd36e7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f8faf6c4c8d9e9c3fecf17749068f030cbbe1d57fcfd66cbb7ea4d9adf459dc1",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2022-12-20T22:39:39Z",
"title_canon_sha256": "45998e7b1f8a8c91100c54d9dabe236a86e32adc0397a0e4be1ec4b58f1ee4a5"
},
"schema_version": "1.0",
"source": {
"id": "2212.10677",
"kind": "arxiv",
"version": 2
}
}