Pith Number
pith:RQOGGGP6
pith:2017:RQOGGGP6NZKZ5SHWEOFVG2Q4GK
not attested
not anchored
not stored
refs pending
Evidence that particle acceleration in hotspots of FR II galaxies is not constrained by synchrotron cooling
arxiv:1703.01193 v1 · 2017-03-03 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RQOGGGP6NZKZ5SHWEOFVG2Q4GK}
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 | 2026-05-18T00:49:35.752058Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8c1c6319fe6e559ec8f6238b536a1c329dfba0d528d1e1e4438df7551e921f37
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RQOGGGP6NZKZ5SHWEOFVG2Q4GK \
| 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: 8c1c6319fe6e559ec8f6238b536a1c329dfba0d528d1e1e4438df7551e921f37
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2f37d6709e755a283416c06a683483c2e2535d6cc9b04dac9b506e71e10b5d1a",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-03-03T15:01:20Z",
"title_canon_sha256": "27a86710928b12dbd277a6cd34e44152f67e19c489db32b9be9c2bef82cfa8d2"
},
"schema_version": "1.0",
"source": {
"id": "1703.01193",
"kind": "arxiv",
"version": 1
}
}