Pith Number
pith:MWIGQY4N
pith:2014:MWIGQY4NCXVUFYSNOGK4MDJ3M3
not attested
not anchored
not stored
refs pending
Magnetic braking of Ap/Bp stars: an alternative formation mechanism of compact intermediate-mass binary pulsars
arxiv:1405.0691 v1 · 2014-05-04 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MWIGQY4NCXVUFYSNOGK4MDJ3M3}
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
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claim
4
Citations
5
Replications
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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 | 2026-05-18T01:43:19.898429Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
659068638d15eb42e24d7195c60d3b66dd1589a12c0feebe3a0e18e0980833c4
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MWIGQY4NCXVUFYSNOGK4MDJ3M3 \
| 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: 659068638d15eb42e24d7195c60d3b66dd1589a12c0feebe3a0e18e0980833c4
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1dbcb6cbc408b84046ae286d918fb074ea437cbc2d1059027c059527b431c984",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2014-05-04T12:39:55Z",
"title_canon_sha256": "79324c74bfff71dd059c2c2586903aa04ec2ae0933d68d1e11e2703539a00a71"
},
"schema_version": "1.0",
"source": {
"id": "1405.0691",
"kind": "arxiv",
"version": 1
}
}