Pith Number
pith:MISRY26C
pith:2017:MISRY26CGTKNM55RMTJKYW3PYF
not attested
not anchored
not stored
refs pending
A Monte Carlo approach to magnetar-powered transients: II. Broad-lined type Ic supernovae not associated with GRBs
arxiv:1702.03156 v2 · 2017-02-10 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MISRY26CGTKNM55RMTJKYW3PYF}
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 | 2026-05-18T00:28:02.445924Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
62251c6bc234d4d677b164d2ac5b6fc17c64876f526d5bbb81c541c815dc17de
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MISRY26CGTKNM55RMTJKYW3PYF \
| 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: 62251c6bc234d4d677b164d2ac5b6fc17c64876f526d5bbb81c541c815dc17de
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "32291b2a3eb6bc61c0062249323350f1c28c960cb29a9a3a3606ff6a933ef0d1",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-02-10T12:58:00Z",
"title_canon_sha256": "431f4e3cc6e2fb48b85774ea7b409f0dd0610d9616fc83642e8e546a49809354"
},
"schema_version": "1.0",
"source": {
"id": "1702.03156",
"kind": "arxiv",
"version": 2
}
}