Pith Number
pith:JWS5LOOU
pith:2023:JWS5LOOUIPNVUJ5UWNHZP2IPU6
not attested
not anchored
not stored
refs pending
KAOSS: turbulent, but disc-like kinematics in dust-obscured star-forming galaxies at $z\sim$1.3-2.6
arxiv:2301.05720 v3 · 2023-01-13 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{JWS5LOOUIPNVUJ5UWNHZP2IPU6}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-07-05T08:13:58.243285Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4da5d5b9d443db5a27b4b34f97e90fa7aa986a50aa9dc9c141665db5310256b6
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/JWS5LOOUIPNVUJ5UWNHZP2IPU6 \
| 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: 4da5d5b9d443db5a27b4b34f97e90fa7aa986a50aa9dc9c141665db5310256b6
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "83569f673e759971c58aea2d9f30173730c5faaf04ac994e8966f0efb1b7408f",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2023-01-13T19:00:02Z",
"title_canon_sha256": "cfa651afe5c1c9275054083b4ee3f8b7052df325a243c6bc37ddb75c036ee466"
},
"schema_version": "1.0",
"source": {
"id": "2301.05720",
"kind": "arxiv",
"version": 3
}
}