Pith Number
pith:YQHOTIYZ
pith:2000:YQHOTIYZRRN4MLIX2EVSQM2EVW
not attested
not anchored
not stored
refs pending
The characteristics of high velocity O and B stars which are ejected from supernovae in binary systems
arxiv:astro-ph/0005021 v1 · 2000-05-01 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YQHOTIYZRRN4MLIX2EVSQM2EVW}
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 | 2026-07-04T16:16:22.709834Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c40ee9a3198c5bc62d17d12b283344ad9410dbfa4391e3c2440b4844c95490bf
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YQHOTIYZRRN4MLIX2EVSQM2EVW \
| 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: c40ee9a3198c5bc62d17d12b283344ad9410dbfa4391e3c2440b4844c95490bf
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f0bc17de3fbf4a29c5923de1726ba38972172fe1781834edc40b05b1ee9e8808",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2000-05-01T16:46:42Z",
"title_canon_sha256": "a4c44e2fede1fd385ecb0b65ea105939eaad7e5bcf64234c9fc5ddc7db5b4606"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0005021",
"kind": "arxiv",
"version": 1
}
}