Pith Number
pith:5TFEYLA6
pith:2014:5TFEYLA6B5COQPNJPTQCIVOCSO
not attested
not anchored
not stored
refs pending
Investigating the magnetic inclination angle distribution of $\gamma$-ray-loud radio pulsars
arxiv:1410.3310 v1 · 2014-10-13 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{5TFEYLA6B5COQPNJPTQCIVOCSO}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:41:48.855321Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ecca4c2c1e0f44e83da97ce02455c29388783a496d3d2e814a4bf11f62079fb0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5TFEYLA6B5COQPNJPTQCIVOCSO \
| 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: ecca4c2c1e0f44e83da97ce02455c29388783a496d3d2e814a4bf11f62079fb0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2f02671329021a581767874b028889f5cf9ca5bb42670bdfa05826ea804a8ecc",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2014-10-13T13:51:09Z",
"title_canon_sha256": "d5a7c90b327c4233de2b38563fd2358a9b8ce428d322c208cad8182810d4b04c"
},
"schema_version": "1.0",
"source": {
"id": "1410.3310",
"kind": "arxiv",
"version": 1
}
}