Pith Number
pith:LXOYKZNP
pith:2019:LXOYKZNPHK3E74VIPRQ4JX4W6I
not attested
not anchored
not stored
refs pending
Ultra-heavy cosmic-ray science--Are r-process nuclei in the cosmic rays produced in supernovae or binary neutron star mergers?
arxiv:1903.12228 v1 · 2019-03-28 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{LXOYKZNPHK3E74VIPRQ4JX4W6I}
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.
Receipt and verification
| First computed | 2026-05-17T23:49:54.531056Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5ddd8565af3ab64ff2a87c61c4df96f212d4af199a9bfeae8526547098cc31df
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/LXOYKZNPHK3E74VIPRQ4JX4W6I \
| 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: 5ddd8565af3ab64ff2a87c61c4df96f212d4af199a9bfeae8526547098cc31df
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2bf4ba2f4dff0ba9e50bd89b1fc1a70726df5b2d65070ff5c39faa9ef2ad2f6e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2019-03-28T19:14:52Z",
"title_canon_sha256": "291f563913c8f4e95dfd7974cb316c87c7a72fe8256b3518dea4f0f322a9a936"
},
"schema_version": "1.0",
"source": {
"id": "1903.12228",
"kind": "arxiv",
"version": 1
}
}