Pith Number
pith:EVAP4ZJO
pith:2013:EVAP4ZJOTGIMYZK4RYXJL4OKZF
not attested
not anchored
not stored
refs pending
The age structure of stellar populations in the solar vicinity. Clues of a two-phase formation history of the Milky Way disk
arxiv:1305.4663 v2 · 2013-05-20 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{EVAP4ZJOTGIMYZK4RYXJL4OKZF}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
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 | 2026-05-18T01:49:48.553379Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2540fe652e9990cc655c8e2e95f1cac97dd65f716a5c1e604bb300bb9dcbe3ff
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EVAP4ZJOTGIMYZK4RYXJL4OKZF \
| 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: 2540fe652e9990cc655c8e2e95f1cac97dd65f716a5c1e604bb300bb9dcbe3ff
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3f8bbc10e35216268cc39bca802a8ca295253a134034d5f3b9ef3a07d7b75189",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2013-05-20T21:20:54Z",
"title_canon_sha256": "2fc67e086f26f2590d96bc55ae046882eb4c1cf3adfeaf38b27a58b922eb476a"
},
"schema_version": "1.0",
"source": {
"id": "1305.4663",
"kind": "arxiv",
"version": 2
}
}