Pith Number
pith:24QSOLWL
pith:2022:24QSOLWLUXBJF6DKWRYK5LWS6R
not attested
not anchored
not stored
refs pending
The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7
arxiv:2208.08243 v2 · 2022-08-17 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{24QSOLWLUXBJF6DKWRYK5LWS6R}
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 | 2026-07-05T05:16:22.455349Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d721272ecba5c292f86ab470aeaed2f44ac8a90fdb105b0bd3b2fd89a2841680
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/24QSOLWLUXBJF6DKWRYK5LWS6R \
| 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: d721272ecba5c292f86ab470aeaed2f44ac8a90fdb105b0bd3b2fd89a2841680
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1d7f234e64083d3af3eeacee7b19181df862ae3959b87e85fac88f7a0ecc6834",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2022-08-17T11:51:17Z",
"title_canon_sha256": "8f65459c89954e55df3a8ec67b4c25676115da2d49a063f5209bdffe66d95c84"
},
"schema_version": "1.0",
"source": {
"id": "2208.08243",
"kind": "arxiv",
"version": 2
}
}