Pith Number
pith:BSXDFIBW
pith:2017:BSXDFIBWDF4P537NECSQL6DGZG
not attested
not anchored
not stored
refs pending
Limits on radial differential rotation in Sun-like stars from parametric fits to oscillation power spectra
arxiv:1705.10517 v1 · 2017-05-30 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BSXDFIBWDF4P537NECSQL6DGZG}
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 | 2026-05-18T00:40:57.514356Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0cae32a0361978feefed20a505f866c9a618977e4e32966f6fc22a5130a0f098
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BSXDFIBWDF4P537NECSQL6DGZG \
| 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: 0cae32a0361978feefed20a505f866c9a618977e4e32966f6fc22a5130a0f098
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "b4a211eabb874ead7f7b28a8be5b66b30e8492aa5eb8df0f874bb3b7685971ba",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2017-05-30T09:23:26Z",
"title_canon_sha256": "fa4a5617274d39c8843ee6d8d293f50d5798f9b40950a7ef9b4c2ac96e7981cd"
},
"schema_version": "1.0",
"source": {
"id": "1705.10517",
"kind": "arxiv",
"version": 1
}
}