Pith Number
pith:CCS2QTSN
pith:2013:CCS2QTSNMXLFHC7NGXEOIY5ORA
not attested
not anchored
not stored
refs pending
What determines the grain size distribution in galaxies?
arxiv:1303.5528 v1 · 2013-03-22 · astro-ph.GA
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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claim
4
Citations
5
Replications
✓
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 | 2026-05-18T01:50:59.625329Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
10a5a84e4d65d6538bed35c8e463ae880353bb176fbd5ddd93d68da22fe67470
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CCS2QTSNMXLFHC7NGXEOIY5ORA \
| 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: 10a5a84e4d65d6538bed35c8e463ae880353bb176fbd5ddd93d68da22fe67470
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f8c21e7639f4b7358d45b58a8a2c912f769d2b8142f81d6d06895229558bf52b",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2013-03-22T06:44:52Z",
"title_canon_sha256": "f3b93cbc45edbeb309699e6613490390f2f904fe3fb763e085215b295a02c900"
},
"schema_version": "1.0",
"source": {
"id": "1303.5528",
"kind": "arxiv",
"version": 1
}
}