Pith Number
pith:KY5EUDHY
pith:2018:KY5EUDHYM37CPB4T6GYYDIZX5S
not attested
not anchored
not stored
refs pending
Is the gamma-ray emission around the Coma galaxy cluster a dark matter origin?
arxiv:1801.01645 v1 · 2018-01-05 · astro-ph.HE · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KY5EUDHYM37CPB4T6GYYDIZX5S}
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 | 2026-05-18T00:26:41.513980Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
563a4a0cf866fe278793f1b181a337ecbf6a2d0e4148320186a3266b3aaea2c7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KY5EUDHYM37CPB4T6GYYDIZX5S \
| 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: 563a4a0cf866fe278793f1b181a337ecbf6a2d0e4148320186a3266b3aaea2c7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3429a6d0ecc3f057f2604a39ff897a7178226740751aad3685bc7ee4d5f5d9ca",
"cross_cats_sorted": [
"hep-ph"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-01-05T06:50:31Z",
"title_canon_sha256": "6c85e167252b5239dbfcfcc373675f1eb19384f3e81c35ee67cf4a76fbf0293c"
},
"schema_version": "1.0",
"source": {
"id": "1801.01645",
"kind": "arxiv",
"version": 1
}
}