Pith Number
pith:KGS53QHS
pith:2017:KGS53QHSATFHHER4B4CL5SFVFN
not attested
not anchored
not stored
refs pending
Characterizing the population of pulsars in the inner Galaxy with the Fermi Large Area Telescope
arxiv:1705.00009 v2 · 2017-04-28 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KGS53QHSATFHHER4B4CL5SFVFN}
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
✓
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 | 2026-05-18T00:31:51.184423Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
51a5ddc0f204ca73923c0f04bec8b52b505b6f5fe32efff586df89064ec48b49
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KGS53QHSATFHHER4B4CL5SFVFN \
| 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: 51a5ddc0f204ca73923c0f04bec8b52b505b6f5fe32efff586df89064ec48b49
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0200d8403fbe414f368457e7d8322afaa9db43d0958087b78a5821199723acc8",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-04-28T18:00:06Z",
"title_canon_sha256": "46489611a6e10c867bb378c345f55d7d78b71d57e2c59f61bcf48d813ca73095"
},
"schema_version": "1.0",
"source": {
"id": "1705.00009",
"kind": "arxiv",
"version": 2
}
}