Pith Number
pith:VCGASQVI
pith:2013:VCGASQVIX5LFXCJ4XMBSX2DCHH
not attested
not anchored
not stored
refs pending
Influence of the cosmic repulsion on the MOND model of the Magellanic Cloud motion in the field of Milky Way
arxiv:1312.0817 v1 · 2013-12-03 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{VCGASQVIX5LFXCJ4XMBSX2DCHH}
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
· 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 | 2026-05-18T01:45:59.207751Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a88c0942a8bf565b893cbb032be86239def9c1460d22a9ad24d3e73b4c23d1c8
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/VCGASQVIX5LFXCJ4XMBSX2DCHH \
| 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: a88c0942a8bf565b893cbb032be86239def9c1460d22a9ad24d3e73b4c23d1c8
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "73e22b39d2c0c491f5af0c7226a1dba2ca8054f1c82d0e1583a010afb64eb626",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2013-12-03T13:30:26Z",
"title_canon_sha256": "c9f94c2ddcf7cd78a1a50ece817a9acde98f4e0bd07af42b010050bfa6686c6a"
},
"schema_version": "1.0",
"source": {
"id": "1312.0817",
"kind": "arxiv",
"version": 1
}
}