Pith Number
pith:MLVHWINX
pith:2017:MLVHWINX6C32ZZJV5NWBBXYAFU
not attested
not anchored
not stored
refs pending
On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
arxiv:1701.05190 v2 · 2017-01-18 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MLVHWINX6C32ZZJV5NWBBXYAFU}
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
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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 | 2026-05-18T00:46:43.972657Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
62ea7b21b7f0b7ace535eb6c10df002d22d6e75dd959f3ba2af4aac186cb2a5b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MLVHWINX6C32ZZJV5NWBBXYAFU \
| 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: 62ea7b21b7f0b7ace535eb6c10df002d22d6e75dd959f3ba2af4aac186cb2a5b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a27356423a8003782a5ffac25e897f5801f0f35fcf1b3526ef9bcbfd8cb1751e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-01-18T19:00:01Z",
"title_canon_sha256": "5a4725885f4eb879c54ea0cd15571aec3f494d578fdbaa7bf33c203f052cfd3d"
},
"schema_version": "1.0",
"source": {
"id": "1701.05190",
"kind": "arxiv",
"version": 2
}
}