Pith Number
pith:WHXBITS7
pith:2010:WHXBITS746FIKNFLSMUBJ642HO
not attested
not anchored
not stored
refs pending
The evolution of luminosity, colour and the mass-to-luminosity ratio of Galactic open clusters: comparison of discrete vs. continuous IMF models
arxiv:1010.2309 v1 · 2010-10-12 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WHXBITS746FIKNFLSMUBJ642HO}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
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Bitcoin timestamp
2
Internet Archive
3
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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 | 2026-05-18T01:09:22.186714Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b1ee144e5fe78a8534ab932814fb9a3b80f29f697921b2ff8419fbe64640cbe3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WHXBITS746FIKNFLSMUBJ642HO \
| 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: b1ee144e5fe78a8534ab932814fb9a3b80f29f697921b2ff8419fbe64640cbe3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "404d47d624ca15f847ae85774d0086a04805cb09188756ebb802db614f4edd36",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2010-10-12T07:30:17Z",
"title_canon_sha256": "3866860ec23d677350649878e5069efbf1cc03ffedd0e8c2c1b8ff8527f16357"
},
"schema_version": "1.0",
"source": {
"id": "1010.2309",
"kind": "arxiv",
"version": 1
}
}