Pith Number
pith:IEZWNK3B
pith:2009:IEZWNK3BTFW3JJO7CAHOQJJTUK
not attested
not anchored
not stored
refs pending
Can X-ray emission powered by a spinning-down magnetar explain some GRB light curve features?
arxiv:0908.3798 v1 · 2009-08-26 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IEZWNK3BTFW3JJO7CAHOQJJTUK}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T02:12:22.786032Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
413366ab61996db4a5df100ee82533a2884176c7d1e33cd9c2ca27e9bcfdad89
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IEZWNK3BTFW3JJO7CAHOQJJTUK \
| 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: 413366ab61996db4a5df100ee82533a2884176c7d1e33cd9c2ca27e9bcfdad89
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1e350126ba3a1bf228bc31700d56afade3cbdc9a61b5dec0ca5f414943286a33",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2009-08-26T12:23:19Z",
"title_canon_sha256": "60d9f739f05f5115050118204bde165dd1afe51ef8bd0f8061550956d2bb5857"
},
"schema_version": "1.0",
"source": {
"id": "0908.3798",
"kind": "arxiv",
"version": 1
}
}