Pith Number
pith:P77HNXPD
pith:2003:P77HNXPD6FN4IPLQABQHSCSDWE
not attested
not anchored
not stored
refs pending
The origin of optical emission from super-Eddington accreting Active Galactic Nuclei: the case of Ton S 180
arxiv:astro-ph/0311266 v1 · 2003-11-12 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{P77HNXPD6FN4IPLQABQHSCSDWE}
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
· sign in to
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 | 2026-07-04T16:37:48.144201Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
7ffe76dde3f15bc43d700060790a43b108352892a02f524197f00cba70922189
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/P77HNXPD6FN4IPLQABQHSCSDWE \
| 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: 7ffe76dde3f15bc43d700060790a43b108352892a02f524197f00cba70922189
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e31bc1ee2344e7e9eaf8c33221390a50903f46d74e106dd71394a4e94526d21f",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2003-11-12T17:38:39Z",
"title_canon_sha256": "531f9498fb2d358607c8a44a98b74ff6c4a9854cdbe3985af18a8585f37dda3c"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0311266",
"kind": "arxiv",
"version": 1
}
}