Pith Number
pith:DAP6GNJL
pith:2012:DAP6GNJLXB3DDE5QWJST25YFG7
not attested
not anchored
not stored
refs pending
Evolution of the Most Massive Galaxies to z ~ 0.6: II. The link between radio AGN activity and star formation
arxiv:1208.1584 v1 · 2012-08-08 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{DAP6GNJLXB3DDE5QWJST25YFG7}
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 | 2026-05-18T01:55:21.943583Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
181fe3352bb8763193b0b2653d770537f7d7d2d7dca4348134c89b697a9521c0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/DAP6GNJLXB3DDE5QWJST25YFG7 \
| 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: 181fe3352bb8763193b0b2653d770537f7d7d2d7dca4348134c89b697a9521c0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "4fa910c5d0ca135d78839236a40020816728a9b65f9876524650035eac4ca527",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2012-08-08T05:32:02Z",
"title_canon_sha256": "5cfbad072bdbd6b6ee64ee63dbf81a571e29376c236edea39a520bed6e2f92bb"
},
"schema_version": "1.0",
"source": {
"id": "1208.1584",
"kind": "arxiv",
"version": 1
}
}