Pith Number
pith:XBP45WIK
pith:2013:XBP45WIKMHLFOGESFLAAMTXVQL
not attested
not anchored
not stored
refs pending
Ultraviolet to infrared emission of z>1 galaxies: Can we derive reliable star formation rates and stellar masses?
arxiv:1310.7712 v1 · 2013-10-29 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XBP45WIKMHLFOGESFLAAMTXVQL}
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 | 2026-05-18T01:46:48.057566Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b85fced90a61d65718922ac0064ef582f09268857448a7b6e6207d9b69cbf052
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XBP45WIKMHLFOGESFLAAMTXVQL \
| 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: b85fced90a61d65718922ac0064ef582f09268857448a7b6e6207d9b69cbf052
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e963649ebe25cea467dc653f736e46d90ea9a40aa312595cfe06197d06dfea58",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2013-10-29T09:06:30Z",
"title_canon_sha256": "c90c6754f53812e70b00e1030299e3404f0ae0312fff6fc19fe3fc9b50aa8f5a"
},
"schema_version": "1.0",
"source": {
"id": "1310.7712",
"kind": "arxiv",
"version": 1
}
}