Pith Number
pith:C7VCWMVR
pith:2011:C7VCWMVR2HMN65M74KZAFTX45U
not attested
not anchored
not stored
refs pending
The role of large-scale magnetic fields in galaxy NGC 891. Can magnetic fields help to reduce the local mass-to-light ratio in the galactic outskirts?
arxiv:1111.6417 v2 · 2011-11-28 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{C7VCWMVR2HMN65M74KZAFTX45U}
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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 | 2026-05-18T03:58:36.725443Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
17ea2b32b1d1d8df759fe2b202cefced070c448d4e912814ed6f18940c522d29
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/C7VCWMVR2HMN65M74KZAFTX45U \
| 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: 17ea2b32b1d1d8df759fe2b202cefced070c448d4e912814ed6f18940c522d29
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8f5d99c91db959365ef2c91dde62ba85c9eb2042f37814f02032292be06dea14",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2011-11-28T11:32:53Z",
"title_canon_sha256": "96ddd78e9925d7b0fd7505fe1cb218f0a5c50ad98f5e45a18148066af61d0211"
},
"schema_version": "1.0",
"source": {
"id": "1111.6417",
"kind": "arxiv",
"version": 2
}
}