Pith Number
pith:KX45N2BC
pith:2025:KX45N2BCQ2H4CBPPSEB6ADJ5E6
not attested
not anchored
not stored
refs pending
The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
arxiv:2501.12008 v2 · 2025-01-21 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KX45N2BCQ2H4CBPPSEB6ADJ5E6}
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
✓
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 | 2026-07-05T10:28:33.281401Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
55f9d6e822868fc105ef9103e00d3d2789f1c8b3b00887a4b99b91159a4d028b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KX45N2BCQ2H4CBPPSEB6ADJ5E6 \
| 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: 55f9d6e822868fc105ef9103e00d3d2789f1c8b3b00887a4b99b91159a4d028b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8036d4f0d2537d4bde90fa16d2ddd7d40ba63e589267d9b34db790b56c94e1a6",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2025-01-21T10:00:46Z",
"title_canon_sha256": "f76323760f7fa5d3d0f648c88486b03bfad714abd45c3f11053cfd7f254bf53b"
},
"schema_version": "1.0",
"source": {
"id": "2501.12008",
"kind": "arxiv",
"version": 2
}
}