Pith Number
pith:RM6D4LZW
pith:2010:RM6D4LZWUY6KOSLSQNS3CVTDIT
not attested
not anchored
not stored
refs pending
Sustaining star formation rates in spiral galaxies - Supernova-driven turbulent accretion disk models applied to THINGS galaxies
arxiv:1009.3722 v1 · 2010-09-20 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RM6D4LZWUY6KOSLSQNS3CVTDIT}
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 | 2026-05-18T02:05:21.690526Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8b3c3e2f36a63ca749728365b1566344eaac91f621147e2669ade15f3190343c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RM6D4LZWUY6KOSLSQNS3CVTDIT \
| 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: 8b3c3e2f36a63ca749728365b1566344eaac91f621147e2669ade15f3190343c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "6df6d93cbf83612e3b8b2710472e8fc2127b59c999f5554a7e0e7cbafc9a657b",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-09-20T07:47:42Z",
"title_canon_sha256": "9c47d946d5b6826f37d17c74611eb519cc0872f44e16d2c60fe5308f26a591c0"
},
"schema_version": "1.0",
"source": {
"id": "1009.3722",
"kind": "arxiv",
"version": 1
}
}