Pith Number
pith:T3BM4Q55
pith:2025:T3BM4Q55DL2FBK6VPLLAZSULMU
not attested
not anchored
not stored
refs pending
Dark matter explanations for the neutrino emission from the Seyfert galaxy NGC 1068
arxiv:2507.16539 v1 · 2025-07-22 · hep-ph · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{T3BM4Q55DL2FBK6VPLLAZSULMU}
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.
Cited by
Receipt and verification
| First computed | 2026-07-05T11:41:11.688056Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
9ec2ce43bd1af450abd57ad60cca8b651104248235a4a71d26c1ccddc76aec0b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/T3BM4Q55DL2FBK6VPLLAZSULMU \
| 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: 9ec2ce43bd1af450abd57ad60cca8b651104248235a4a71d26c1ccddc76aec0b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e2bbcc36a69c533a5e3928012ef3fbd995958fc7275035025ac679525a58f73e",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "hep-ph",
"submitted_at": "2025-07-22T12:49:13Z",
"title_canon_sha256": "f48ab250c549ed85a9c8d9a5b1ebfb55eb4f3d757d606a3851713d046d85d0fd"
},
"schema_version": "1.0",
"source": {
"id": "2507.16539",
"kind": "arxiv",
"version": 1
}
}