Pith Number
pith:CEHMGMBD
pith:2019:CEHMGMBDHNIVGR25DGUZVWMXQZ
not attested
not anchored
not stored
refs pending
Evidence for the accretion origin of halo stars with an extreme r-process enhancement
arxiv:1905.04141 v1 · 2019-05-10 · astro-ph.SR · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{CEHMGMBDHNIVGR25DGUZVWMXQZ}
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 | 2026-05-17T23:46:34.408683Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
110ec330233b5153475d19a99ad9978673ba85eb41db3c7a3844e25cf84c0ca7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CEHMGMBDHNIVGR25DGUZVWMXQZ \
| 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: 110ec330233b5153475d19a99ad9978673ba85eb41db3c7a3844e25cf84c0ca7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dc7d74f33e8828eccad276100cdd2137474477ca69666a3093098900268fa80e",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2019-05-10T12:54:20Z",
"title_canon_sha256": "255f1fa179ab4ad3258702985de2bf26fe3aece4e364cd484de86c0b9bd766b7"
},
"schema_version": "1.0",
"source": {
"id": "1905.04141",
"kind": "arxiv",
"version": 1
}
}