Pith Number
pith:YTXD35WR
pith:2002:YTXD35WR2IBZOS7Z7OMUHXQLK6
not attested
not anchored
not stored
refs pending
High Mass X-ray Binaries as a Star Formation Rate Indicator in Distant Galaxies
arxiv:astro-ph/0205371 v2 · 2002-05-22 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YTXD35WR2IBZOS7Z7OMUHXQLK6}
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.
Cited by
Receipt and verification
| First computed | 2026-07-04T16:30:03.352690Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c4ee3df6d1d203974bf9fb9943de0b578ae808c18db534739082bcb27febf442
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YTXD35WR2IBZOS7Z7OMUHXQLK6 \
| 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: c4ee3df6d1d203974bf9fb9943de0b578ae808c18db534739082bcb27febf442
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "4001766bbe835307ae93be499d0985f2dfe2a1077759f2fdcd05c3c5be092851",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2002-05-22T14:33:19Z",
"title_canon_sha256": "110836f456b15668b19602ab1ad24cedebbc1fe165eb3353f05d684f02c0cc73"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0205371",
"kind": "arxiv",
"version": 2
}
}