Pith Number
pith:WGYZ26I3
pith:2017:WGYZ26I3ZAHCU3ZXVMVWIEQVE5
not attested
not anchored
not stored
refs pending
UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles
arxiv:1705.05404 v1 · 2017-05-15 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WGYZ26I3ZAHCU3ZXVMVWIEQVE5}
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 | 2026-05-18T00:44:22.799994Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b1b19d791bc80e2a6f37ab2b641215275b07f2fa59180617c9ea35769a4e49bc
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WGYZ26I3ZAHCU3ZXVMVWIEQVE5 \
| 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: b1b19d791bc80e2a6f37ab2b641215275b07f2fa59180617c9ea35769a4e49bc
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "49790ac89fa759ca9d9f77e45da9b9adebb984ba87ab9497abecb42ccd40e415",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-05-15T18:23:43Z",
"title_canon_sha256": "2d01e9b983473415f163e784e0d397d3fca7aca3ba6bedd5f3ec274d26a1cd81"
},
"schema_version": "1.0",
"source": {
"id": "1705.05404",
"kind": "arxiv",
"version": 1
}
}