Pith Number
pith:WXXHFV3D
pith:2014:WXXHFV3DCSC7D62G4EQG34RBOV
not attested
not anchored
not stored
refs pending
How does a low-mass cut-off in the stellar IMF affect the evolution of young star clusters?
arxiv:1409.2613 v1 · 2014-09-09 · astro-ph.SR · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WXXHFV3DCSC7D62G4EQG34RBOV}
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 | 2026-05-18T01:42:06.214754Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b5ee72d7631485f1fb46e1206df2217551795f741293fe5d99852f74fc708652
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WXXHFV3DCSC7D62G4EQG34RBOV \
| 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: b5ee72d7631485f1fb46e1206df2217551795f741293fe5d99852f74fc708652
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "edcb423f28a85f3c86f4044acb7edb40371f4cb96f8798e56a37434e275a3e85",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2014-09-09T06:32:36Z",
"title_canon_sha256": "f3d84f232fafbc395740dd3c6912149e190265df035132d1d0813f0172823df2"
},
"schema_version": "1.0",
"source": {
"id": "1409.2613",
"kind": "arxiv",
"version": 1
}
}