Pith Number
pith:5LVHDJYE
pith:2011:5LVHDJYEOBHSU2NLCSM52722FP
not attested
not anchored
not stored
refs pending
Magnetars vs. high magnetic field pulsars: a theoretical interpretation of the apparent dichotomy
arxiv:1109.5184 v1 · 2011-09-23 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{5LVHDJYEOBHSU2NLCSM52722FP}
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 | 2026-05-18T03:59:13.769090Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
eaea71a704704f2a69ab1499dd7f5a2bfe57ab2c7b5fcb4fda3f53588a624569
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5LVHDJYEOBHSU2NLCSM52722FP \
| 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: eaea71a704704f2a69ab1499dd7f5a2bfe57ab2c7b5fcb4fda3f53588a624569
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f3d53263b53124a30ac3050db9d43771ff0894e01f101b62a1502d31285aa0f5",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2011-09-23T20:00:32Z",
"title_canon_sha256": "7c167be78daa2d8b6997afa9541f62b4b30c86a950d7a665b005e9545fcf81e7"
},
"schema_version": "1.0",
"source": {
"id": "1109.5184",
"kind": "arxiv",
"version": 1
}
}