Pith Number
pith:6CYMR26L
pith:2019:6CYMR26LAEFHX7BY3IPHPMACQS
not attested
not anchored
not stored
refs pending
Modelling the distributions of white dwarf atmospheric pollution: a low Mg abundance for accreted planetesimals?
arxiv:1911.05131 v1 · 2019-11-12 · astro-ph.EP · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{6CYMR26LAEFHX7BY3IPHPMACQS}
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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 | 2026-07-05T00:27:45.313208Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
f0b0c8ebcb010a7bfc38da1e77b002848de03c12a95585cef5baf0e56e49d099
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/6CYMR26LAEFHX7BY3IPHPMACQS \
| 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: f0b0c8ebcb010a7bfc38da1e77b002848de03c12a95585cef5baf0e56e49d099
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8a8b8487d26a35dcc250f43721b680d218d1ec8b86f5f5c663607345296b8dbe",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.EP",
"submitted_at": "2019-11-12T20:35:58Z",
"title_canon_sha256": "30149d2f333b1c56baefedff8e48d11e51ec66d9431323ed6a7689c6a0c0d48a"
},
"schema_version": "1.0",
"source": {
"id": "1911.05131",
"kind": "arxiv",
"version": 1
}
}