Pith Number
pith:3XN3WVF5
pith:2024:3XN3WVF5R55OXS6MKBMQJHVXHC
not attested
not anchored
not stored
refs pending
SKA Sensitivity to Potential Radio Emission from Dark Matter Annihilation in Ursa Major III
arxiv:2409.12414 v1 · 2024-09-19 · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{3XN3WVF5R55OXS6MKBMQJHVXHC}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-07-05T09:08:53.707422Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
dddbbb54bd8f7aebcbcc5059049eb738b7555a0cfb8c354057ec5deffe8d1637
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3XN3WVF5R55OXS6MKBMQJHVXHC \
| 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: dddbbb54bd8f7aebcbcc5059049eb738b7555a0cfb8c354057ec5deffe8d1637
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cc793e53c6eb54ba9a4fd7bde8135cf706f137992136a82c408848ca5505384e",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "hep-ph",
"submitted_at": "2024-09-19T02:24:24Z",
"title_canon_sha256": "5ceed4eeaff4d77ad0e1c0909347757b8513053b52534b094b7ce77cc96c74fa"
},
"schema_version": "1.0",
"source": {
"id": "2409.12414",
"kind": "arxiv",
"version": 1
}
}