Pith Number
pith:GWSYV67Z
pith:2023:GWSYV67ZTXPG5BORVXFTD7HRUF
not attested
not anchored
not stored
refs pending
An observational upper limit on the rate of gamma-ray bursts with neutron star-black hole merger progenitors
arxiv:2306.14974 v1 · 2023-06-26 · astro-ph.HE · gr-qc
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GWSYV67ZTXPG5BORVXFTD7HRUF}
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 | 2026-07-05T06:47:02.248652Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
35a58afbf99dde6e85d1adcb31fcf1a16235fd11845de5807a2394b82393b3e0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GWSYV67ZTXPG5BORVXFTD7HRUF \
| 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: 35a58afbf99dde6e85d1adcb31fcf1a16235fd11845de5807a2394b82393b3e0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5f046e63ddfa930ba80e3ecd2939a5c01aaf7e90c442c09479750bb14f987406",
"cross_cats_sorted": [
"gr-qc"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2023-06-26T18:01:27Z",
"title_canon_sha256": "0fb5b25fb21514b341bdbb683e889b7d017a4baf54cc97d99e4afb395aed6165"
},
"schema_version": "1.0",
"source": {
"id": "2306.14974",
"kind": "arxiv",
"version": 1
}
}