Pith Number
pith:NUG24VBI
pith:2015:NUG24VBIMU4T2666MHJ4HI3AX6
not attested
not anchored
not stored
refs pending
The Biases of Optical Line-Ratio Selection for Active Galactic Nuclei, and the Intrinsic Relationship between Black Hole Accretion and Galaxy Star Formation
arxiv:1501.02801 v3 · 2015-01-12 · astro-ph.GA
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\usepackage{pith}
\pithnumber{NUG24VBIMU4T2666MHJ4HI3AX6}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:32:30.367084Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
6d0dae542865393d7bde61d3c3a360bf9f0a35726463391de2065536cc3427c4
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/NUG24VBIMU4T2666MHJ4HI3AX6 \
| 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: 6d0dae542865393d7bde61d3c3a360bf9f0a35726463391de2065536cc3427c4
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0b5b9773d78305006ab935a1ef763a76a9aa05a6b2a9507b9ffc17f666ad00b7",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2015-01-12T21:00:11Z",
"title_canon_sha256": "6cd20771da513d7308b75c77a86dd6bde71ad904474e3cdb438108c926642037"
},
"schema_version": "1.0",
"source": {
"id": "1501.02801",
"kind": "arxiv",
"version": 3
}
}