Pith Number
pith:KDUYMMNT
pith:2016:KDUYMMNTLJHQO4KN2L4ISGWYVZ
not attested
not anchored
not stored
refs pending
A New Maximum-Likelihood Technique for Reconstructing Cosmic-Ray Anisotropy at All Angular Scales
arxiv:1601.07877 v2 · 2016-01-28 · astro-ph.HE · hep-ex
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KDUYMMNTLJHQO4KN2L4ISGWYVZ}
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
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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 | 2026-05-18T01:14:35.597218Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
50e98631b35a4f07714dd2f8891ad8ae52340d9181fa74dc2f732084c4e8a32e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KDUYMMNTLJHQO4KN2L4ISGWYVZ \
| 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: 50e98631b35a4f07714dd2f8891ad8ae52340d9181fa74dc2f732084c4e8a32e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5b14e2a02b4c5755a49a3236ea5723285fe06e550acaeb7630e55bfcccbc406a",
"cross_cats_sorted": [
"hep-ex"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2016-01-28T19:40:07Z",
"title_canon_sha256": "d015a97cdd10716d9282af53807246f115dd37c62734ae8b715c76d680ca7c46"
},
"schema_version": "1.0",
"source": {
"id": "1601.07877",
"kind": "arxiv",
"version": 2
}
}