Pith Number
pith:CXU5EAVX
pith:2009:CXU5EAVXT7SQ3NT32F7Q47ISVQ
not attested
not anchored
not stored
refs pending
The relationship between star formation rate and radio synchrotron luminosity at 0 < z < 2
arxiv:0905.1218 v1 · 2009-05-08 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{CXU5EAVXT7SQ3NT32F7Q47ISVQ}
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 | 2026-05-18T02:13:46.442962Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
15e9d202b79fe50db67bd17f0e7d12ac2bc5e97634e5fe656fb084edc024fef8
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CXU5EAVXT7SQ3NT32F7Q47ISVQ \
| 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: 15e9d202b79fe50db67bd17f0e7d12ac2bc5e97634e5fe656fb084edc024fef8
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e5ae644d3ebd6ca6f67524a2716577d81fcdc03d533d6a6b02276888a17deca5",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2009-05-08T10:39:45Z",
"title_canon_sha256": "bdb4b4065f271968f6052037944633b2795111b287bf1514218f59ddaa8482c2"
},
"schema_version": "1.0",
"source": {
"id": "0905.1218",
"kind": "arxiv",
"version": 1
}
}