Pith Number
pith:I3RYUTL5
pith:2020:I3RYUTL5UNJAP4P6K2XULPPUTE
not attested
not anchored
not stored
refs pending
Physically constrained causal noise models for high-contrast imaging of exoplanets
arxiv:2010.05591 v2 · 2020-10-12 · astro-ph.IM · cs.LG
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{I3RYUTL5UNJAP4P6K2XULPPUTE}
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 | 2026-07-05T01:58:12.263369Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
46e38a4d7da35207f1fe56af45bdf4993b93ea41c8ee4d6b0bc3b93948be231f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/I3RYUTL5UNJAP4P6K2XULPPUTE \
| 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: 46e38a4d7da35207f1fe56af45bdf4993b93ea41c8ee4d6b0bc3b93948be231f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "692f1f1a8a47e2549b4add838733ad6db66f1ed87ca3d5fc00e163682c2643f9",
"cross_cats_sorted": [
"cs.LG"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.IM",
"submitted_at": "2020-10-12T10:35:03Z",
"title_canon_sha256": "c2ffc643b39524911abc415650ed3e312f9b9b57df6792145426fbaf86ce3530"
},
"schema_version": "1.0",
"source": {
"id": "2010.05591",
"kind": "arxiv",
"version": 2
}
}