Pith Number
pith:H2BEBYNW
pith:2011:H2BEBYNW3E3SCMPWYYHYMDKYTV
not attested
not anchored
not stored
refs pending
Two distinct halo populations in the solar neighborhood. II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
arxiv:1103.4755 v1 · 2011-03-24 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{H2BEBYNW3E3SCMPWYYHYMDKYTV}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T02:02:47.377389Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3e8240e1b6d9372131f6c60f860d589d45faecc7a137ad76ea64ba012cf9d0aa
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/H2BEBYNW3E3SCMPWYYHYMDKYTV \
| 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: 3e8240e1b6d9372131f6c60f860d589d45faecc7a137ad76ea64ba012cf9d0aa
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7a14657d603ecb490b5c020ee03e10675e34993dfbe4a1e7a4d57ca66962b02f",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2011-03-24T12:54:19Z",
"title_canon_sha256": "78320a5272e642b501d0dc7df75946d9fda8c27ce76ce0b90501be2960b3cfca"
},
"schema_version": "1.0",
"source": {
"id": "1103.4755",
"kind": "arxiv",
"version": 1
}
}