Pith Number
pith:CG5SRLTO
pith:2024:CG5SRLTOOYLSDD4OY2H3XBGMB7
not attested
not anchored
not stored
refs pending
The impact of large-scale galaxy clustering on the variance of the Hellings-Downs correlation: theoretical framework
arxiv:2404.05670 v2 · 2024-04-08 · astro-ph.CO · gr-qc
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{CG5SRLTOOYLSDD4OY2H3XBGMB7}
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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.
Cited by
Exploring the statistical anisotropy of primordial curvature perturbations with pulsar timing arrays
Receipt and verification
| First computed | 2026-07-05T10:26:02.250732Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
11bb28ae6e7617218f8ec68fbb84cc0fc832e38c585edc2beef500045be1819a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CG5SRLTOOYLSDD4OY2H3XBGMB7 \
| 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: 11bb28ae6e7617218f8ec68fbb84cc0fc832e38c585edc2beef500045be1819a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f197c09ef2c3e491edff36f9acab2891d9c14b9ede7d1f976c7b42d2972875dc",
"cross_cats_sorted": [
"gr-qc"
],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2024-04-08T16:53:12Z",
"title_canon_sha256": "91f95e978168303671e38ba3b8fa35fbc33c4d222018e523d2de7de87482e706"
},
"schema_version": "1.0",
"source": {
"id": "2404.05670",
"kind": "arxiv",
"version": 2
}
}