Pith Number
pith:2X6LRP4L
pith:2010:2X6LRP4LP4IODDU2LZK4CGL76N
not attested
not anchored
not stored
refs pending
A comparison of spectroscopic methods for detecting starlight scattered by transiting hot Jupiters, with application to Subaru data for HD 209458b and HD 189733b
arxiv:1006.5492 v2 · 2010-06-29 · astro-ph.EP
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{2X6LRP4LP4IODDU2LZK4CGL76N}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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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 | 2026-05-18T02:06:34.644707Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d5fcb8bf8b7f10e18e9a5e55c1197ff34431c31f6b3c68b6da7672efd0bbbad6
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2X6LRP4LP4IODDU2LZK4CGL76N \
| 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: d5fcb8bf8b7f10e18e9a5e55c1197ff34431c31f6b3c68b6da7672efd0bbbad6
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "65ea2fd31b1e06925bd3f58ced339d0a0098cd8beca01b5ad39e6805f9ba94a6",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.EP",
"submitted_at": "2010-06-29T02:21:10Z",
"title_canon_sha256": "82edb873c23fe23d3f40fc67795ba03b4690ad4c0e8039782650cdf7072e3cf9"
},
"schema_version": "1.0",
"source": {
"id": "1006.5492",
"kind": "arxiv",
"version": 2
}
}