Pith Number
pith:EHNFKTBD
pith:2010:EHNFKTBDXIDAXUOISIQO6EIQ2I
not attested
not anchored
not stored
refs pending
The black holes of radio galaxies during the "Quasar Era": Masses, accretion rates, and evolutionary stage
arxiv:1011.4158 v1 · 2010-11-18 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{EHNFKTBDXIDAXUOISIQO6EIQ2I}
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 | 2026-05-18T02:04:44.077883Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
21da554c23ba060bd1c89220ef1110d2311648e1bc180bcc93dde59e3d28d30f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EHNFKTBDXIDAXUOISIQO6EIQ2I \
| 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: 21da554c23ba060bd1c89220ef1110d2311648e1bc180bcc93dde59e3d28d30f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5ae7107c4317496a2e357f927a237593c4733e0413f15aa95defb7c8c733c6bc",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-11-18T09:15:44Z",
"title_canon_sha256": "6f2754b0963b1b6239cfa3b2ce4f27df0564a71aa40c757256087b8967396d55"
},
"schema_version": "1.0",
"source": {
"id": "1011.4158",
"kind": "arxiv",
"version": 1
}
}