Pith Number
pith:O2YPRWPW
pith:2011:O2YPRWPWLPSUEKEP7XB3EO3RPN
not attested
not anchored
not stored
refs pending
Implications of high-precision spectra of thermonuclear X-ray bursts for determining neutron star masses and radii
arxiv:1105.2030 v2 · 2011-05-10 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{O2YPRWPWLPSUEKEP7XB3EO3RPN}
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 | 2026-05-18T04:19:21.526917Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
76b0f8d9f65be542288ffdc3b23b717b65cf2d4590f81810da7a4c59f8dfd90e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/O2YPRWPWLPSUEKEP7XB3EO3RPN \
| 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: 76b0f8d9f65be542288ffdc3b23b717b65cf2d4590f81810da7a4c59f8dfd90e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "aa7edf60d4551adba9cbfb1ce1771708b7b14e4bf4515becafc9d5e52bbb5631",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2011-05-10T19:46:39Z",
"title_canon_sha256": "27716e117d06d4b3fe28340789605d26b217b42421ff5cc9e3680543eec7fbda"
},
"schema_version": "1.0",
"source": {
"id": "1105.2030",
"kind": "arxiv",
"version": 2
}
}