Pith Number
pith:3Q2TPRQU
pith:2018:3Q2TPRQUCXEE47NZIAKNQD32AI
not attested
not anchored
not stored
refs pending
On the rates of type Ia supernovae originating from white dwarf collisions in quadruple star systems
arxiv:1804.05847 v1 · 2018-04-16 · astro-ph.SR · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3Q2TPRQUCXEE47NZIAKNQD32AI}
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 | 2026-05-18T00:17:03.134912Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
dc3537c61415c84e7db94014d80f7a02180383a54cb4e4861d83ca165427a9f7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3Q2TPRQUCXEE47NZIAKNQD32AI \
| 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: dc3537c61415c84e7db94014d80f7a02180383a54cb4e4861d83ca165427a9f7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "ae6410b128c3abbb15fce69f8563469cef7179732f518004af8f86baaddee6eb",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2018-04-16T18:00:02Z",
"title_canon_sha256": "4110270c158c0839d0f5a6612fc264bc9829d7fec370bc413008716b9af5dbd8"
},
"schema_version": "1.0",
"source": {
"id": "1804.05847",
"kind": "arxiv",
"version": 1
}
}