Pith Number
pith:2BBE23T5
pith:2004:2BBE23T5J6T4FL6CPTQLRX7NV4
not attested
not anchored
not stored
refs pending
A robust sample of submillimetre galaxies: constraints on the prevalence of dusty, high-redshift starbursts
arxiv:astro-ph/0412084 v3 · 2004-12-03 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{2BBE23T5J6T4FL6CPTQLRX7NV4}
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 | 2026-07-04T16:45:20.936471Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d0424d6e7d4fa7c2afc27ce0b8dfedaf0e4bfd58db9b631f7b152a7aca1584ff
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2BBE23T5J6T4FL6CPTQLRX7NV4 \
| 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: d0424d6e7d4fa7c2afc27ce0b8dfedaf0e4bfd58db9b631f7b152a7aca1584ff
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "6de7d4c44ec649659c1b9a292ecc4b74a3014ee6fffade9ac559adb167bda0ba",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2004-12-03T17:31:38Z",
"title_canon_sha256": "303cb2bc7fb222c35d61f252d0eabf80126d85dd008b48b91912c64e8163bda7"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0412084",
"kind": "arxiv",
"version": 3
}
}