Pith Number
pith:4H672RPK
pith:2014:4H672RPKOQ355ZAWFPYFS4XWTI
not attested
not anchored
not stored
refs pending
The stability of stellar disks in Milky-Way sized dark matter halos
arxiv:1411.3729 v2 · 2014-11-13 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4H672RPKOQ355ZAWFPYFS4XWTI}
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
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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 | 2026-05-18T01:36:58.201516Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e1fdfd45ea7437dee4162bf05972f69a33d851c685cbb8c5effe514f1a78d1c0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4H672RPKOQ355ZAWFPYFS4XWTI \
| 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: e1fdfd45ea7437dee4162bf05972f69a33d851c685cbb8c5effe514f1a78d1c0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "58b17eef9435848c0c9b59afac95207c16e9b195556f89c24a51d13fc13fc823",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-11-13T21:00:08Z",
"title_canon_sha256": "027c8da77e9fe8ab378acb7b50a6d821b364fb746c1b5e4326a64199488c2a8b"
},
"schema_version": "1.0",
"source": {
"id": "1411.3729",
"kind": "arxiv",
"version": 2
}
}