Pith Number
pith:7CUGC47E
pith:2017:7CUGC47EXFURJFBM6R2UW44S56
not attested
not anchored
not stored
refs pending
Does the radial-tangential macroturbulence model adequately describe the spectral line broadening of solar-type stars?
arxiv:1703.02233 v1 · 2017-03-07 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{7CUGC47EXFURJFBM6R2UW44S56}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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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 | 2026-05-18T00:42:06.991580Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
f8a86173e4b96914942cf4754b7392ef9c40d1df80354ca518a101e3e26ad4c0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/7CUGC47EXFURJFBM6R2UW44S56 \
| 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: f8a86173e4b96914942cf4754b7392ef9c40d1df80354ca518a101e3e26ad4c0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "df5a2b1556a05f12278823b435e581d5d31b6503813d3fc63ac9d848d56034cb",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2017-03-07T06:26:43Z",
"title_canon_sha256": "79cefbcb9435f6c1e74faadd58b0c2d8fb5d9d3298c4369dd734eb986532f767"
},
"schema_version": "1.0",
"source": {
"id": "1703.02233",
"kind": "arxiv",
"version": 1
}
}