Pith Number
pith:5M7Q2XKT
pith:2015:5M7Q2XKTPK4Y3KP4ETYSD4L7BG
not attested
not anchored
not stored
refs pending
The link between accretion mode and environment in radio-loud active galaxies
arxiv:1508.01033 v2 · 2015-08-05 · astro-ph.GA · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{5M7Q2XKTPK4Y3KP4ETYSD4L7BG}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:32:59.433280Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
eb3f0d5d537ab98da9fc24f121f17f09a11aa8763c2dcaceb50730b33aae54e4
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5M7Q2XKTPK4Y3KP4ETYSD4L7BG \
| 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: eb3f0d5d537ab98da9fc24f121f17f09a11aa8763c2dcaceb50730b33aae54e4
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "07216c3a77fa718285219508ffb9a7dda298168c7a15eff23b57d717bc835872",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2015-08-05T10:39:41Z",
"title_canon_sha256": "c3afc8327fd0aeb671fd22dbab4e5a3c746c55638a3f8cec683aca7e425d3d88"
},
"schema_version": "1.0",
"source": {
"id": "1508.01033",
"kind": "arxiv",
"version": 2
}
}