Pith Number
pith:AGXEU54G
pith:2017:AGXEU54GNL63JKVRJEPPKHSCGN
not attested
not anchored
not stored
refs pending
Can winds driven by active galactic nuclei account for the extragalactic gamma-ray and neutrino backgrounds?
arxiv:1712.10168 v2 · 2017-12-29 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{AGXEU54GNL63JKVRJEPPKHSCGN}
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 | 2026-05-18T00:17:10.994397Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
01ae4a77866afdb4aab1491ef51e42334e2d60e015d7c790d28ff39c1b10feef
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/AGXEU54GNL63JKVRJEPPKHSCGN \
| 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: 01ae4a77866afdb4aab1491ef51e42334e2d60e015d7c790d28ff39c1b10feef
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dad4cbde26875a3b759432b8de36c42a1433afa935786d12aa9e8de1984e5a02",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-12-29T10:30:15Z",
"title_canon_sha256": "ff6520645950949c986bf865566c4a8f3bc87e72aa6c0662a517ddd5f972f380"
},
"schema_version": "1.0",
"source": {
"id": "1712.10168",
"kind": "arxiv",
"version": 2
}
}