Pith Number
pith:XFL5KGGI
pith:2010:XFL5KGGIT23NRAEHNAI7SASRAB
not attested
not anchored
not stored
refs pending
The Prevalence of Narrow Optical Fe II Emission Lines in Type 1 Active Galactic Nuclei
arxiv:1009.2209 v1 · 2010-09-12 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XFL5KGGIT23NRAEHNAI7SASRAB}
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 | 2026-05-18T04:41:04.587851Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b957d518c89eb6d880876811f902510062d498c5abaf487c78f550fb5db82722
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XFL5KGGIT23NRAEHNAI7SASRAB \
| 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: b957d518c89eb6d880876811f902510062d498c5abaf487c78f550fb5db82722
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "70411a41eabf04b9db4714c0de97f7494fce02c60f065a6ead50b6992dbc7755",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2010-09-12T01:08:07Z",
"title_canon_sha256": "7eeed7f7e1bcacc02d883424302a6d2a9fc7b6bccb0cadc8bed468cb53b9976a"
},
"schema_version": "1.0",
"source": {
"id": "1009.2209",
"kind": "arxiv",
"version": 1
}
}