Pith Number
pith:RBA5W5LM
pith:2010:RBA5W5LMOXJKLUTK2VPBFXBVC6
not attested
not anchored
not stored
refs pending
Missing Power vs low-l Alignments in the Cosmic Microwave Background: No Correlation in the Standard Cosmological Model
arxiv:1004.3784 v1 · 2010-04-21 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RBA5W5LMOXJKLUTK2VPBFXBVC6}
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 | 2026-05-18T02:07:55.512367Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8841db756c75d2a5d26ad55e12dc3517a1d5769f1f51fcd6040ccfb71f25a274
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RBA5W5LMOXJKLUTK2VPBFXBVC6 \
| 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: 8841db756c75d2a5d26ad55e12dc3517a1d5769f1f51fcd6040ccfb71f25a274
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a2b353896dee278fa3913d4b77d19b2655b1bfcf0277cf6edfb2c4e84d4b6bcf",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-04-21T20:00:01Z",
"title_canon_sha256": "340d885541c9b659e6f0acb8085f020571e1aa94f2a6d3904600b5374bacb7b6"
},
"schema_version": "1.0",
"source": {
"id": "1004.3784",
"kind": "arxiv",
"version": 1
}
}