Pith Number
pith:K6MHCPSO
pith:2016:K6MHCPSONN2QYLENRTWVOD4I3T
not attested
not anchored
not stored
refs pending
A high fraction of Be stars in young massive clusters: evidence for a large population of near-critically rotating stars
arxiv:1611.06705 v1 · 2016-11-21 · astro-ph.GA
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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4
Citations
5
Replications
Receipt and verification
| First computed | 2026-05-18T00:53:06.696740Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519 (pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5798713e4e6b750c2c8d8ced570f88dcceafdfb653182b26d8948b7187ef885a
Aliases
· ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/K6MHCPSONN2QYLENRTWVOD4I3T \
| 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: 5798713e4e6b750c2c8d8ced570f88dcceafdfb653182b26d8948b7187ef885a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8b0d619388fc0da1dbcaaf0d1d57016401b19b38b3fbcd127150672cb0bd119f",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2016-11-21T10:04:30Z",
"title_canon_sha256": "f351edad392afe32a3889f489bfb9c1c72fa5dc93ab7d6462bb5f6e1281784d0"
},
"schema_version": "1.0",
"source": {
"id": "1611.06705",
"kind": "arxiv",
"version": 1
}
}