Pith Number
pith:JMY3ORJV
pith:2010:JMY3ORJVJLFYUIXXXHHMXHLQWK
not attested
not anchored
not stored
refs pending
The Accreting Millisecond X-ray Pulsar IGR J00291+5934: Evidence for a Long Timescale Spin Evolution
arxiv:1006.0815 v2 · 2010-06-04 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{JMY3ORJVJLFYUIXXXHHMXHLQWK}
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 | 2026-05-18T02:07:04.820810Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4b31b745354acb8a22f7b9cecb9d70b294f6d5419d86c08e6cf647f791ed8b12
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/JMY3ORJVJLFYUIXXXHHMXHLQWK \
| 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: 4b31b745354acb8a22f7b9cecb9d70b294f6d5419d86c08e6cf647f791ed8b12
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a21bc835a9c61e38291ce5e307293f3c0e3e74b83972b8460febb3281dcdbb3e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2010-06-04T09:20:30Z",
"title_canon_sha256": "b27a749c96de30b4911495867d0fcdbfe48e0ffffcbc6dc2c717e1d43e869c78"
},
"schema_version": "1.0",
"source": {
"id": "1006.0815",
"kind": "arxiv",
"version": 2
}
}