Pith Number
pith:LMCSEE3H
pith:2022:LMCSEE3HP2Y3ZX4HFB4BB3ZH47
not attested
not anchored
not stored
refs pending
Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white-dwarfs
arxiv:2201.03827 v2 · 2022-01-11 · astro-ph.SR · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{LMCSEE3HP2Y3ZX4HFB4BB3ZH47}
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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.
Cited by
Receipt and verification
| First computed | 2026-07-05T03:52:34.516271Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5b052213677eb1bcdf87287810ef27e7e18323695b4372ee077b3243c33a01ac
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/LMCSEE3HP2Y3ZX4HFB4BB3ZH47 \
| 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: 5b052213677eb1bcdf87287810ef27e7e18323695b4372ee077b3243c33a01ac
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "b792f3324b1e9928c3a312b69618edee55f9edf82ebc77cef32fcdaddc59fc44",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2022-01-11T08:14:40Z",
"title_canon_sha256": "a58c456c4f96583d5d49ba4d6d6491931e804d5fd53d835ca8ae03d35c6fb879"
},
"schema_version": "1.0",
"source": {
"id": "2201.03827",
"kind": "arxiv",
"version": 2
}
}