Pith Number
pith:W3E6M5MY
pith:2010:W3E6M5MYXCCPAIEYIXU6ACIKCB
not attested
not anchored
not stored
refs pending
Improved constraints on cosmic microwave background secondary anisotropies from the complete 2008 South Pole Telescope data
arxiv:1012.4788 v2 · 2010-12-21 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{W3E6M5MYXCCPAIEYIXU6ACIKCB}
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 | 2026-05-18T02:23:06.684852Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b6c9e67598b884f0209845e9e0090a107310c2e5983390ce7ab6e5f8f5d8eb04
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/W3E6M5MYXCCPAIEYIXU6ACIKCB \
| 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: b6c9e67598b884f0209845e9e0090a107310c2e5983390ce7ab6e5f8f5d8eb04
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "4945434f03240b7d497e3afe613b24e4858962a874913750e1982fbade0a641e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-12-21T20:43:11Z",
"title_canon_sha256": "ab0b7944b6f6c805122c8a57f1a457c330624ba8917877a9d0f18a6e78d5474e"
},
"schema_version": "1.0",
"source": {
"id": "1012.4788",
"kind": "arxiv",
"version": 2
}
}