Pith Number
pith:BX2IHD2A
pith:2012:BX2IHD2AF6HPKW55YWW33YHDOB
not attested
not anchored
not stored
refs pending
Origin of strong magnetic fields in Milky-Way like galactic haloes
arxiv:1202.3349 v1 · 2012-02-15 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BX2IHD2AF6HPKW55YWW33YHDOB}
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 | 2026-05-18T01:58:28.021427Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0df4838f402f8ef55bbdc5adbde0e3704b99a4b89e2f81848ee77756a6fa9367
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BX2IHD2AF6HPKW55YWW33YHDOB \
| 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: 0df4838f402f8ef55bbdc5adbde0e3704b99a4b89e2f81848ee77756a6fa9367
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "583505f3ccc3cc71d07ad2cbecdf214313d7d29ec3dfb9f4e32cf78938596ba3",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2012-02-15T16:05:16Z",
"title_canon_sha256": "9bb97522ed35733f729a5c795988718b7535ae539f74727454386a35a0f825c3"
},
"schema_version": "1.0",
"source": {
"id": "1202.3349",
"kind": "arxiv",
"version": 1
}
}