Pith Number
pith:4PVYC6GD
pith:2019:4PVYC6GDVYVRQQVBVAO5FQNNL6
not attested
not anchored
not stored
refs pending
Supermassive black holes with high accretion rates in active galactic nuclei: X. Optical variability characteristics
arxiv:1904.03393 v2 · 2019-04-06 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4PVYC6GDVYVRQQVBVAO5FQNNL6}
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
✓
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 | 2026-05-17T23:44:54.594730Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e3eb8178c3ae2b1842a1a81dd2c1ad5fb604609c5e3f3a8ed45102a76e162703
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4PVYC6GDVYVRQQVBVAO5FQNNL6 \
| 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: e3eb8178c3ae2b1842a1a81dd2c1ad5fb604609c5e3f3a8ed45102a76e162703
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cbb02d63ece2ada64c5b06abafc43c5d68294283856884b9ba477e3943bc8d0e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2019-04-06T09:21:05Z",
"title_canon_sha256": "b8e1b393474982436796955913f0e967ac2e33eaf5b63061a933c2fb8b2bdc3b"
},
"schema_version": "1.0",
"source": {
"id": "1904.03393",
"kind": "arxiv",
"version": 2
}
}