Pith Number
pith:FNRQMXZG
pith:2003:FNRQMXZGEHW3ECPJU3RN2KO2I3
not attested
not anchored
not stored
refs pending
Evidence for high accretion-rates in Weak-Line T Tauri stars?
arxiv:astro-ph/0310173 v1 · 2003-10-07 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{FNRQMXZGEHW3ECPJU3RN2KO2I3}
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 | 2026-05-18T01:07:33.262366Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2b63065f2621edb209e9a6e2dd29da46fb6031294f54839be58413175b04b6e6
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/FNRQMXZGEHW3ECPJU3RN2KO2I3 \
| 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: 2b63065f2621edb209e9a6e2dd29da46fb6031294f54839be58413175b04b6e6
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a13a51b50090ca6308052f3e63de306b978c33cae5e1291c3f31b7d6da92aaa2",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2003-10-07T13:36:06Z",
"title_canon_sha256": "bbb61cf7a8c97abb752a03d3122281d4ab4ae00444ed7e221b1ea557c1f9b7c0"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0310173",
"kind": "arxiv",
"version": 1
}
}