Pith Number
pith:ISBAUBYV
pith:2013:ISBAUBYVMFFT2T6KBQ5ZEWSNT4
not attested
not anchored
not stored
refs pending
Do radio magnetars J1550-5418 and J1622-4950 have gigahertz-peaked spectra?
arxiv:1305.5346 v1 · 2013-05-23 · astro-ph.SR · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{ISBAUBYVMFFT2T6KBQ5ZEWSNT4}
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 | 2026-05-18T01:49:47.412889Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
44820a0715614b3d4fca0c3b925a4d9f130a90adb841b57812680e10ccd8d108
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/ISBAUBYVMFFT2T6KBQ5ZEWSNT4 \
| 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: 44820a0715614b3d4fca0c3b925a4d9f130a90adb841b57812680e10ccd8d108
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "c34391e08495904b1960dc248ee2b7e6fecf92243e4e45fb97478ec3189d604f",
"cross_cats_sorted": [
"astro-ph.HE"
],
"license": "http://creativecommons.org/licenses/by-nc-sa/3.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2013-05-23T08:48:17Z",
"title_canon_sha256": "dcde662b90b36e4f95932fedb8964df4b84ae157b530abc3c323a1adbf9492e2"
},
"schema_version": "1.0",
"source": {
"id": "1305.5346",
"kind": "arxiv",
"version": 1
}
}