Pith Number
pith:H7AVBFMX
pith:2017:H7AVBFMXU2KBDRDVFCOMBSY2OP
not attested
not anchored
not stored
refs pending
Does the evolution of the radio luminosity function of star-forming galaxies match that of the star-formation rate function?
arxiv:1704.05459 v2 · 2017-04-18 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{H7AVBFMXU2KBDRDVFCOMBSY2OP}
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 | 2026-05-18T00:42:04.704791Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3fc1509597a69411c475289cc0cb1a73f8af064ce24a998ca114b8e5c070446f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/H7AVBFMXU2KBDRDVFCOMBSY2OP \
| 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: 3fc1509597a69411c475289cc0cb1a73f8af064ce24a998ca114b8e5c070446f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3fb4dc548abdbdbe3ad544d2d6e726e3bde1b0ae28a8e9ddd36dfde29b269e62",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-04-18T18:00:01Z",
"title_canon_sha256": "34b80ee110088a94809e0796723b235556b7a2bd187d97f1ac175e74b41565ef"
},
"schema_version": "1.0",
"source": {
"id": "1704.05459",
"kind": "arxiv",
"version": 2
}
}