Pith Number
pith:IIVSLYQH
pith:2011:IIVSLYQHVHCRAMS66PKOF4SNSB
not attested
not anchored
not stored
refs pending
Variable X-ray emission from the accretion shock in the Classical T Tauri Star V2129 Oph
arxiv:1102.5751 v1 · 2011-02-28 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IIVSLYQHVHCRAMS66PKOF4SNSB}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T02:03:02.171425Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
422b25e207a9c510325ef3d4e2f24d904598a8eb4de7a7b43151e75bf969e8b5
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IIVSLYQHVHCRAMS66PKOF4SNSB \
| 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: 422b25e207a9c510325ef3d4e2f24d904598a8eb4de7a7b43151e75bf969e8b5
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "54b432ba9668a085ffae70c44eaaeadc1a3d253a42eaf065d3493633ed6f90b6",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2011-02-28T19:33:15Z",
"title_canon_sha256": "cdbf52d3dd3ee2fddcec1e0bcaf794042dc2f80f4071ff4c6dd999dec37243d3"
},
"schema_version": "1.0",
"source": {
"id": "1102.5751",
"kind": "arxiv",
"version": 1
}
}