Pith Number
pith:4GSG3GMU
pith:2018:4GSG3GMU5EC7YTHKB33OXMMFFP
not attested
not anchored
not stored
refs pending
What fraction of the density fluctuations in the Perseus cluster core is due to gas sloshing rather than AGN feedback?
arxiv:1808.10460 v1 · 2018-08-30 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4GSG3GMU5EC7YTHKB33OXMMFFP}
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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 | 2026-05-18T00:06:00.897467Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e1a46d9994e905fc4cea0ef6ebb1852bd6750b6d9f99562bf8e27608bce9d66c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4GSG3GMU5EC7YTHKB33OXMMFFP \
| 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: e1a46d9994e905fc4cea0ef6ebb1852bd6750b6d9f99562bf8e27608bce9d66c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "c1af35e40bdadd469a9ab7287af6f94bce287b6929b037f3f2287af00bef7560",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-08-30T18:00:09Z",
"title_canon_sha256": "d4e0665b22cf4d094f269d9ee4a086d6c224aedae0098f4128389de29ea35205"
},
"schema_version": "1.0",
"source": {
"id": "1808.10460",
"kind": "arxiv",
"version": 1
}
}