Pith Number
pith:5Q3FX3SC
pith:2018:5Q3FX3SCTWW745F5X5SHZWHXXU
not attested
not anchored
not stored
refs pending
A lower occurrence rate of bright X-ray flares in SN-GRBs than $z<1$ GRBs: evidence of energy partitions?
arxiv:1805.05722 v1 · 2018-05-15 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{5Q3FX3SCTWW745F5X5SHZWHXXU}
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 | 2026-05-18T00:14:07.441028Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ec365bee429dadfe74bdbf647cd8f7bd3c0abf61e3eb3519c69f7f8fe9621261
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5Q3FX3SCTWW745F5X5SHZWHXXU \
| 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: ec365bee429dadfe74bdbf647cd8f7bd3c0abf61e3eb3519c69f7f8fe9621261
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2ec3d73782055fcdb7f853ef0333bab3bc3ef3f11fac408687bd3699e15b708b",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-05-15T12:08:53Z",
"title_canon_sha256": "466c4f88cb9117b4109d97a3e32a2282341d85ab9e458f4d69a30fcab75fc09b"
},
"schema_version": "1.0",
"source": {
"id": "1805.05722",
"kind": "arxiv",
"version": 1
}
}