Pith Number
pith:T7KNHGKL
pith:2001:T7KNHGKLMN2WGJUOD44CZWYL2R
not attested
not anchored
not stored
refs pending
Faraday Rotation Effect of Intracluster Magnetic Field on Cosmic Microwave Background Polarization
arxiv:astro-ph/0112412 v1 · 2001-12-17 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{T7KNHGKLMN2WGJUOD44CZWYL2R}
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 | 2026-07-04T14:11:43.937727Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
9fd4d3994b637563268e1f382cdb0bd455fd48ee57e97cee00c4debed799b197
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/T7KNHGKLMN2WGJUOD44CZWYL2R \
| 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: 9fd4d3994b637563268e1f382cdb0bd455fd48ee57e97cee00c4debed799b197
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a7e220acb26257719ea33df13f7f948970d0d77f9b79d2e4678c99154b444005",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2001-12-17T23:42:38Z",
"title_canon_sha256": "dea682917a561cfda195e50f09665efe9eef6b5d63fe6c3363ee8d9706ae1cde"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0112412",
"kind": "arxiv",
"version": 1
}
}