Pith Number
pith:OS5NTREI
pith:2015:OS5NTREIHS2YWVYCCV6P2ER42M
not attested
not anchored
not stored
refs pending
The Structure of Nuclear Star Clusters in Nearby Late-type Spiral Galaxies from Hubble Space Telescope Wide Field Camera 3 Imaging
arxiv:1501.05586 v2 · 2015-01-22 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OS5NTREIHS2YWVYCCV6P2ER42M}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
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 | 2026-05-18T01:41:09.247513Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
74bad9c4883cb58b5702157cfd123cd31720d31a9b17e191bf6f51f2cd890b96
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OS5NTREIHS2YWVYCCV6P2ER42M \
| 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: 74bad9c4883cb58b5702157cfd123cd31720d31a9b17e191bf6f51f2cd890b96
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "c4b19d60e7dbb9df8b8a497668d43b673eb3a4b9a21b0ab45e120c575fddfe4b",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2015-01-22T17:54:20Z",
"title_canon_sha256": "4996baaff3dc87eb811af9c99f84e196dc45d9e8ec413b467e24d225af69496a"
},
"schema_version": "1.0",
"source": {
"id": "1501.05586",
"kind": "arxiv",
"version": 2
}
}