Pith Number
pith:XAEXV5RF
pith:2003:XAEXV5RF2VZ5YGSBHETNBJQ4W5
not attested
not anchored
not stored
refs pending
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources
arxiv:astro-ph/0305097 v1 · 2003-05-07 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XAEXV5RF2VZ5YGSBHETNBJQ4W5}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T04:22:19.771430Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b8097af625d573dc1a413926d0a61cb7578a83626f71aff8532ad166365144af
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XAEXV5RF2VZ5YGSBHETNBJQ4W5 \
| 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: b8097af625d573dc1a413926d0a61cb7578a83626f71aff8532ad166365144af
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "922ce15f0dc00b114695327ef9fe2c901d2beba1cf382ec7abd9b2b82326bfc7",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2003-05-07T05:33:36Z",
"title_canon_sha256": "27a5eac156ed567a193349a236c2b80a2a8b034f084f5a5624fd2834901d2c1e"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0305097",
"kind": "arxiv",
"version": 1
}
}