Pith Number
pith:ZGSWLRA5
pith:2013:ZGSWLRA5AG7I2YK2YBWEA7XXHJ
not attested
not anchored
not stored
refs pending
The initial mass function of star clusters that form in turbulent molecular clouds
arxiv:1309.1223 v3 · 2013-09-05 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{ZGSWLRA5AG7I2YK2YBWEA7XXHJ}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:47:49.601817Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c9a565c41d01be8d615ac06c407ef73a7db18ef925379f6361d86df5b787f90f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/ZGSWLRA5AG7I2YK2YBWEA7XXHJ \
| 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: c9a565c41d01be8d615ac06c407ef73a7db18ef925379f6361d86df5b787f90f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d5ca7d9c3dc4ca1590637b9494a997028a17c3c792dc623913678c735afe787e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2013-09-05T02:05:57Z",
"title_canon_sha256": "d321b1df28f5a5699a7937ea2b8a3c25a428d9b6c063fc75de2f7361e9415b98"
},
"schema_version": "1.0",
"source": {
"id": "1309.1223",
"kind": "arxiv",
"version": 3
}
}