Pith Number
pith:6PR6CMDC
pith:2008:6PR6CMDCC7RHEBW64PAEO2WYBN
not attested
not anchored
not stored
refs pending
The Contribution of Radio Selected Star Forming Galaxies to the IR Energy Density Budget
arxiv:0805.0773 v1 · 2008-05-06 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{6PR6CMDCC7RHEBW64PAEO2WYBN}
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 | 2026-07-04T15:11:23.757616Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
f3e3e1306217e27206dee3c0476ad80b48ddcf1ffdc6a6e0fbf677584b61a67f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/6PR6CMDCC7RHEBW64PAEO2WYBN \
| 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: f3e3e1306217e27206dee3c0476ad80b48ddcf1ffdc6a6e0fbf677584b61a67f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "aad67629eda1382745fd632b6aed79c887f4611e9a50efe123abaf4017cff9ad",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph",
"submitted_at": "2008-05-06T18:36:53Z",
"title_canon_sha256": "5065b7ec6db936ef493f39fc3fda409904db34ef5f916ea420cdbc9d0893ab4c"
},
"schema_version": "1.0",
"source": {
"id": "0805.0773",
"kind": "arxiv",
"version": 1
}
}