Pith Number
pith:Y5WB3JAZ
pith:2024:Y5WB3JAZLHJHNVCYTTW2JLM6AV
not attested
not anchored
not stored
refs pending
Metallicity distributions of halo stars: do they trace the Galactic accretion history?
arxiv:2401.13737 v2 · 2024-01-24 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{Y5WB3JAZLHJHNVCYTTW2JLM6AV}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
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 | 2026-07-05T09:17:06.440590Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c76c1da41959d276d4589ceda4ad9e056437d0933d389af42272cceb3fdcff1d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Y5WB3JAZLHJHNVCYTTW2JLM6AV \
| 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: c76c1da41959d276d4589ceda4ad9e056437d0933d389af42272cceb3fdcff1d
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0d0e1814bf948c8656ad571f9e05c3966631acf7ea434f1a4333c989346df159",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2024-01-24T19:00:02Z",
"title_canon_sha256": "9fe57c322caae2d0564a14c86358bd34edf874aaccde1e91e2c1d0039bf149ef"
},
"schema_version": "1.0",
"source": {
"id": "2401.13737",
"kind": "arxiv",
"version": 2
}
}