Pith Number
pith:HB72EUEE
pith:2026:HB72EUEEZ5OSZ3IQVJDAYED5UC
not attested
not anchored
not stored
refs pending
Cyclotron lines in subcritical X-ray pulsars: Monte Carlo simulations reveal the origin of the observed variability
arxiv:2602.02733 v1 · 2026-02-02 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HB72EUEEZ5OSZ3IQVJDAYED5UC}
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 | 2026-05-27T14:06:40.699751Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
387fa25084cf5d2ced10aa460c107da0af2999ea3b9414e57c296391cb72ce5f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HB72EUEEZ5OSZ3IQVJDAYED5UC \
| 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: 387fa25084cf5d2ced10aa460c107da0af2999ea3b9414e57c296391cb72ce5f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2f188327b2f4a8424dd64adf7c43012c29acdb54a1e32a0583db88ca39304827",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2026-02-02T19:48:08Z",
"title_canon_sha256": "f3ac2841d2572933b0b3900bbc1315c85ab33f7b2f9301f6e27e716437fda267"
},
"schema_version": "1.0",
"source": {
"id": "2602.02733",
"kind": "arxiv",
"version": 1
}
}