Pith Number
pith:4H5SNERG
pith:2019:4H5SNERG44GBBJPH6QXD3JZEPO
not attested
not anchored
not stored
refs pending
Non-Gaussianity in the Weak Lensing Correlation Function Likelihood -- Implications for Cosmological Parameter Biases
arxiv:1905.03779 v2 · 2019-05-09 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4H5SNERG44GBBJPH6QXD3JZEPO}
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 | 2026-07-05T01:50:15.036711Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e1fb269226e70c10a5e7f42e3da7247bbf46ad6752f3e4d7c17cc335bb07b68f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4H5SNERG44GBBJPH6QXD3JZEPO \
| 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: e1fb269226e70c10a5e7f42e3da7247bbf46ad6752f3e4d7c17cc335bb07b68f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "336f37cb9f0cf6bdad421cd35486a7d222158fe90712790966859f636f612797",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2019-05-09T17:59:02Z",
"title_canon_sha256": "5af9d3ea1e79cca29dea6173619c612099db4e83f8b47ab1fc443c475811ea87"
},
"schema_version": "1.0",
"source": {
"id": "1905.03779",
"kind": "arxiv",
"version": 2
}
}