Pith Number
pith:WTWDW3TR
pith:2023:WTWDW3TRQ3PAADM36LC5KHUPIH
not attested
not anchored
not stored
refs pending
A$^3$COSMOS: the infrared luminosity function and dust-obscured star formation rate density at $0.5<z<6$
arxiv:2309.15150 v1 · 2023-09-26 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WTWDW3TRQ3PAADM36LC5KHUPIH}
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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 | 2026-07-05T06:54:41.929872Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b4ec3b6e7186de000d9bf2c5d51e8f41d530f96626c28389ed74743726d4cc6a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WTWDW3TRQ3PAADM36LC5KHUPIH \
| 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: b4ec3b6e7186de000d9bf2c5d51e8f41d530f96626c28389ed74743726d4cc6a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "75b42df6fc286f87fa7c1cef717d03eded80168063548245b9028712d791ab26",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2023-09-26T18:00:03Z",
"title_canon_sha256": "9931dfff0463e12254d00ccffc8515aa664e55147da39b3ed0c41289ddbbdbad"
},
"schema_version": "1.0",
"source": {
"id": "2309.15150",
"kind": "arxiv",
"version": 1
}
}