Pith Number
pith:JW2CMVCU
pith:2024:JW2CMVCUTNTOESQRVSE635MT26
not attested
not anchored
not stored
refs pending
The MAGPI Survey: Using kinematic asymmetries in stars and gas to dissect drivers of galaxy dynamical evolution
arxiv:2405.11292 v1 · 2024-05-18 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{JW2CMVCUTNTOESQRVSE635MT26}
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 | 2026-07-05T08:20:36.611556Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4db42654549b66e24a11ac89edf593d7a6fca585a820c42d820f252781426984
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/JW2CMVCUTNTOESQRVSE635MT26 \
| 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: 4db42654549b66e24a11ac89edf593d7a6fca585a820c42d820f252781426984
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7038068b7a8b60fd5f078dc01d7559373915b8b0a06585010bed46250e8de4d4",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2024-05-18T13:37:11Z",
"title_canon_sha256": "1f9a5023e9a1faab23d31d925824e1f596dcc40e08e416f995d0d56a15644bee"
},
"schema_version": "1.0",
"source": {
"id": "2405.11292",
"kind": "arxiv",
"version": 1
}
}