Pith Number
pith:DWHUE6ID
pith:2014:DWHUE6IDQQNVELW4FPVTXUBG5T
not attested
not anchored
not stored
refs pending
Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3
arxiv:1410.7398 v3 · 2014-10-27 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{DWHUE6IDQQNVELW4FPVTXUBG5T}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T02:27:18.241904Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
1d8f427903841b522edc2beb3bd026ecdd4a7be5e4c99713859c747898bf8ae2
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/DWHUE6IDQQNVELW4FPVTXUBG5T \
| 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: 1d8f427903841b522edc2beb3bd026ecdd4a7be5e4c99713859c747898bf8ae2
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f4365499b9078a45e680823f7793627a253f7d9260652291355f0ad49a39f453",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-10-27T20:00:14Z",
"title_canon_sha256": "7a6eb8119f9f88950b8b8ab92da3599cd8d57b5dc1776fe0ffe87a9aa5087d75"
},
"schema_version": "1.0",
"source": {
"id": "1410.7398",
"kind": "arxiv",
"version": 3
}
}