Pith Number
pith:XJXROKYW
pith:2024:XJXROKYW67A5EE6FGOQVV62OHN
not attested
not anchored
not stored
refs pending
Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
arxiv:2411.00103 v1 · 2024-10-31 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XJXROKYW67A5EE6FGOQVV62OHN}
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.
Cited by
Receipt and verification
| First computed | 2026-07-05T12:07:36.629487Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ba6f172b16f7c1d213c533a15afb4e3b561dd712fcb68315435749372abee9f0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XJXROKYW67A5EE6FGOQVV62OHN \
| 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: ba6f172b16f7c1d213c533a15afb4e3b561dd712fcb68315435749372abee9f0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "136f7aea67fcb1a09fc6a957e0d3f9b7dd0a854f4eeb9081c11b75ad0b6110f0",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2024-10-31T18:00:19Z",
"title_canon_sha256": "70f987e9bd2398d79476a165080af96f3d6f13bc3eabe1f7046ef92a22c1b3a0"
},
"schema_version": "1.0",
"source": {
"id": "2411.00103",
"kind": "arxiv",
"version": 1
}
}