Pith Number
pith:5RXHGP7J
pith:2004:5RXHGP7JMHWLGYK33V3LTTC45G
not attested
not anchored
not stored
refs pending
Do star formation rates of galaxy clusters depend on mass?: blue/late-type fractions, total star formation rates of 115 galaxy clusters as a function of cluster virial mass
arxiv:astro-ph/0411517 v2 · 2004-11-17 · astro-ph
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\usepackage{pith}
\pithnumber{5RXHGP7JMHWLGYK33V3LTTC45G}
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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 | 2026-05-18T01:07:31.908997Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ec6e733fe961ecb3615bdd76b9cc5ce982fa113d08dec5607b23311fd4d62cc3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5RXHGP7JMHWLGYK33V3LTTC45G \
| 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: ec6e733fe961ecb3615bdd76b9cc5ce982fa113d08dec5607b23311fd4d62cc3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2de5855099f725aba1316397546811c205730e1945fb2b4a73db49b65ebf0035",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2004-11-17T22:05:59Z",
"title_canon_sha256": "1cbbc0162f7b781eec6afd34335dbdbeb39571ba46816723476eb38ca472968d"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0411517",
"kind": "arxiv",
"version": 2
}
}