Pith Number
pith:XI2P25AP
pith:2013:XI2P25APSQWCUWP746AWR6I7UU
not attested
not anchored
not stored
refs pending
Near-infrared adaptive optics imaging of infrared luminous galaxies: the brightest cluster magnitude - star formation rate relation
arxiv:1308.6293 v1 · 2013-08-28 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XI2P25APSQWCUWP746AWR6I7UU}
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 | 2026-05-18T01:47:57.187092Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ba34fd740f942c2a59ffe78168f91fa51455c5f7459901ecb236b09a8031403a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XI2P25APSQWCUWP746AWR6I7UU \
| 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: ba34fd740f942c2a59ffe78168f91fa51455c5f7459901ecb236b09a8031403a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "523a52f520d5da75689bd38f4c4ed781868847449d42ea6e9d1e156580a39fe6",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2013-08-28T20:05:22Z",
"title_canon_sha256": "e10ae4bbab5ab1964f488830fb3f4b382049fba65039222e72035ef68bc0b390"
},
"schema_version": "1.0",
"source": {
"id": "1308.6293",
"kind": "arxiv",
"version": 1
}
}