Pith Number
pith:B2FRNUVM
pith:2018:B2FRNUVMJYWDADBSQIK2KFSLPH
not attested
not anchored
not stored
refs pending
The time evolution of the Milky Way's oxygen abundance gradient
arxiv:1810.09182 v1 · 2018-10-22 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{B2FRNUVMJYWDADBSQIK2KFSLPH}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T00:01:57.259412Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0e8b16d2ac4e2c300c328215a5164b79cfdc6a1402cdb704034c5b06b636c32b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/B2FRNUVMJYWDADBSQIK2KFSLPH \
| 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: 0e8b16d2ac4e2c300c328215a5164b79cfdc6a1402cdb704034c5b06b636c32b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7e20948491cf4baaecc2a6809243e7f5558919b936d88aadc04a4f2cbd933a5b",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2018-10-22T11:30:31Z",
"title_canon_sha256": "a2d9642d8aa3bd7b83eaf4db71c161bcf7cd464e0f6c245e2c3c46c34b88b11d"
},
"schema_version": "1.0",
"source": {
"id": "1810.09182",
"kind": "arxiv",
"version": 1
}
}