Pith Number
pith:3HFJ437W
pith:2018:3HFJ437W2EXVUSNIX5L7G324TO
not attested
not anchored
not stored
refs pending
Understanding the $\gamma$-ray emission from the globular cluster 47 Tuc: evidence for dark matter?
arxiv:1806.01866 v1 · 2018-06-05 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3HFJ437W2EXVUSNIX5L7G324TO}
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 | 2026-05-18T00:08:14.705887Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d9ca9e6ff6d12f5a49a8bf57f36f5c9b9a1ad8433183ea137427958c6e9c1669
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3HFJ437W2EXVUSNIX5L7G324TO \
| 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: d9ca9e6ff6d12f5a49a8bf57f36f5c9b9a1ad8433183ea137427958c6e9c1669
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "6b64e87e23d4aa3a9bf814a28356157e2d350e458168755e771a635880ec52ee",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-06-05T18:00:39Z",
"title_canon_sha256": "0b8ac349a38de504c333ba05f581152d921667b077b02e5f547878567fa63ee3"
},
"schema_version": "1.0",
"source": {
"id": "1806.01866",
"kind": "arxiv",
"version": 1
}
}