Pith Number
pith:FHBLYTUL
pith:2011:FHBLYTULWQEE73MIP7TTCTZDIM
not attested
not anchored
not stored
refs pending
The relation between surface star formation rate density and spiral arms in NGC 5236 (M83)
arxiv:1111.1249 v1 · 2011-11-04 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{FHBLYTULWQEE73MIP7TTCTZDIM}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T01:59:45.236956Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
29c2bc4e8bb4084fed887fe7314f23433b71711d00fe3f7ae3f3de07655d9641
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/FHBLYTULWQEE73MIP7TTCTZDIM \
| 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: 29c2bc4e8bb4084fed887fe7314f23433b71711d00fe3f7ae3f3de07655d9641
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "c9c39dd6a20a856c7d057fb094fb38be41fdef49389214517ac9093106e09658",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2011-11-04T21:00:00Z",
"title_canon_sha256": "439a7adb435fc56d461900e7de89dccd36d0f20fdaf63f05d146710a671738aa"
},
"schema_version": "1.0",
"source": {
"id": "1111.1249",
"kind": "arxiv",
"version": 1
}
}