Pith Number
pith:MZ7WWJFG
pith:2005:MZ7WWJFGBPT7KVNHYX422RJRPD
not attested
not anchored
not stored
refs pending
Shapiro Effect as a Possible Cause of the Low-Frequency Pulsar Timing Noise in Globular Clusters
arxiv:astro-ph/0512400 v1 · 2005-12-15 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MZ7WWJFGBPT7KVNHYX422RJRPD}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
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Bitcoin timestamp
2
Internet Archive
3
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4
Citations
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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 | 2026-05-18T01:07:25.623721Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
667f6b24a60be7f555a7c5f9ad453178c2eb58478ed1c4190b49608072c7507c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MZ7WWJFGBPT7KVNHYX422RJRPD \
| 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: 667f6b24a60be7f555a7c5f9ad453178c2eb58478ed1c4190b49608072c7507c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "9dce423195b2b91b7db5524a339da81aacc474040645efbe4fb2ca1f1b601b50",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2005-12-15T15:05:37Z",
"title_canon_sha256": "7f3d4a25379407ced604bad2540fcec84578f5cc591b61642bf48528509025ac"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0512400",
"kind": "arxiv",
"version": 1
}
}