Pith Number
pith:OSHPPGLV
pith:2015:OSHPPGLV46DBW3IGJO7V7CSLFK
not attested
not anchored
not stored
refs pending
The SAMI Galaxy Survey: Can we trust aperture corrections to predict star formation?
arxiv:1510.06038 v1 · 2015-10-20 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OSHPPGLV46DBW3IGJO7V7CSLFK}
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 | 2026-05-18T01:25:38.031100Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
748ef79975e7861b6d064bbf5f8a4b2aac3d904b662c72ca5429bb254e3e50cc
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OSHPPGLV46DBW3IGJO7V7CSLFK \
| 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: 748ef79975e7861b6d064bbf5f8a4b2aac3d904b662c72ca5429bb254e3e50cc
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "b36a2b53a481f5ddde4e998fdd1a6ac7841092ab10e8cb1398ceb7a41f7b3346",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2015-10-20T20:09:31Z",
"title_canon_sha256": "79a37d1842e91e41929ed0c4c9e83b9bbcf88f3d094a59da8d0fc842f11d8340"
},
"schema_version": "1.0",
"source": {
"id": "1510.06038",
"kind": "arxiv",
"version": 1
}
}