Pith Number
pith:22K4TXY2
pith:2010:22K4TXY27DOZ2CVHJ5LL3KROCE
not attested
not anchored
not stored
refs pending
The supernova delay time distribution in galaxy clusters and implications for Type-Ia progenitors and metal enrichment
arxiv:1006.3576 v3 · 2010-06-17 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{22K4TXY27DOZ2CVHJ5LL3KROCE}
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 | 2026-05-18T02:06:44.798798Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d695c9df1af8dd9d0aa74f56bdaa2e110ad131e78cd3f8954eb0807e061a83c3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/22K4TXY27DOZ2CVHJ5LL3KROCE \
| 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: d695c9df1af8dd9d0aa74f56bdaa2e110ad131e78cd3f8954eb0807e061a83c3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "342351b8c45688fc68b88c3fd1afcf2e7d1e0eb6f0a8ad306955e8ddf6d457b1",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-06-17T22:06:08Z",
"title_canon_sha256": "6922a96476ad45f0fd0a3120005a2d29a83794be054fb0671c07e61368252f84"
},
"schema_version": "1.0",
"source": {
"id": "1006.3576",
"kind": "arxiv",
"version": 3
}
}