Pith Number
pith:XKMVUYGL
pith:2016:XKMVUYGLKQWSEPV3ON36FU42WU
not attested
not anchored
not stored
refs pending
Evidence that the maximum electron energy in hotspots of FR II galaxies is not determined by synchrotron cooling
arxiv:1605.05125 v1 · 2016-05-17 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XKMVUYGLKQWSEPV3ON36FU42WU}
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 | 2026-05-18T01:13:10.915915Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ba995a60cb542d223ebb7377e2d39ab53f44e96abcac8c0a7f53868136b8a6e6
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XKMVUYGLKQWSEPV3ON36FU42WU \
| 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: ba995a60cb542d223ebb7377e2d39ab53f44e96abcac8c0a7f53868136b8a6e6
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "30b1c66723369fbee14eb05c6224e7e48cbe583450d35bf13079f87257eed848",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2016-05-17T12:08:34Z",
"title_canon_sha256": "94179f088f1207a0f15197a49fb1753c36136a362b24696a9e8502545e2aa5ff"
},
"schema_version": "1.0",
"source": {
"id": "1605.05125",
"kind": "arxiv",
"version": 1
}
}