Pith Number
pith:H2GXNWAP
pith:2012:H2GXNWAPKQC7R26FAKEKEBAVMQ
not attested
not anchored
not stored
refs pending
Early X-ray and optical afterglow of gravitational wave bursts from mergers of binary neutron stars
arxiv:1212.0773 v2 · 2012-12-04 · astro-ph.HE · gr-qc
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{H2GXNWAPKQC7R26FAKEKEBAVMQ}
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
✓
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:52:47.836338Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3e8d76d80f5405f8ebc50288a2041564136dcb7a794e9589977b4eea4175b49b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/H2GXNWAPKQC7R26FAKEKEBAVMQ \
| 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: 3e8d76d80f5405f8ebc50288a2041564136dcb7a794e9589977b4eea4175b49b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "bfa3908fbc66a3d1df14688a5558ee53f4a64f7d94d4ae129f45a997124afdc7",
"cross_cats_sorted": [
"gr-qc"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2012-12-04T15:54:49Z",
"title_canon_sha256": "a67417e9f7cb7f7472f67cb2af6c538bc197da73e6f9e2b5a2031d34292bac7a"
},
"schema_version": "1.0",
"source": {
"id": "1212.0773",
"kind": "arxiv",
"version": 2
}
}