Pith Number
pith:MVOMOZ5E
pith:2015:MVOMOZ5EYH53AXDB456BZYAKJ6
not attested
not anchored
not stored
refs pending
A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars
arxiv:1601.00004 v2 · 2015-12-31 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MVOMOZ5EYH53AXDB456BZYAKJ6}
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 | 2026-05-18T01:22:05.512564Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
655cc767a4c1fbb05c61e77c1ce00a4f9d1ec7528496c1bca8fa0304ea941fd9
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MVOMOZ5EYH53AXDB456BZYAKJ6 \
| 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: 655cc767a4c1fbb05c61e77c1ce00a4f9d1ec7528496c1bca8fa0304ea941fd9
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d0728835dca86e2dd4272c0ec47c14f9b20c345d6774a2fc81badde652c0d572",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2015-12-31T21:00:03Z",
"title_canon_sha256": "c1a7f9c26dcd23327e5450db2e32b7e2935c108791c1c6b67ee11bd0177340a7"
},
"schema_version": "1.0",
"source": {
"id": "1601.00004",
"kind": "arxiv",
"version": 2
}
}