Pith Number
pith:UYA5MKRN
pith:2011:UYA5MKRNNMZFE5G7NADKVIWTNK
not attested
not anchored
not stored
refs pending
Near-Infrared Spectroscopy of TW Hya: A Revised Spectral Type and Comparison with Magnetospheric Accretion Models
arxiv:1102.0535 v1 · 2011-02-02 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{UYA5MKRNNMZFE5G7NADKVIWTNK}
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 | 2026-05-18T02:03:17.446729Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a601d62a2d6b325274df6806aaa2d36a82188e9f6fd566fd46330df0245f2c24
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UYA5MKRNNMZFE5G7NADKVIWTNK \
| 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: a601d62a2d6b325274df6806aaa2d36a82188e9f6fd566fd46330df0245f2c24
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "38d09d45d508253cbac04710988ac5c8f81febd043d0d13df7301c3f54a95dde",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2011-02-02T19:27:18Z",
"title_canon_sha256": "205ad2d5947a0753423e93bb532d66b4d9a4d8884c0e0f5ef8a13a8f6dd2208f"
},
"schema_version": "1.0",
"source": {
"id": "1102.0535",
"kind": "arxiv",
"version": 1
}
}