Pith Number
pith:BKGSIN75
pith:2010:BKGSIN753KRO7DLZXWZ7SRHOBH
not attested
not anchored
not stored
refs pending
Measuring star formation in high-z massive galaxies: A mid-infrared to submillimeter study of the GOODS NICMOS Survey sample
arxiv:1008.4359 v4 · 2010-08-25 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BKGSIN753KRO7DLZXWZ7SRHOBH}
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 | 2026-05-18T02:05:42.729202Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
0a8d2437fddaa2ef8d79bdb3f944ee09c97d1727526b77b193f5b6e07460ff5b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BKGSIN753KRO7DLZXWZ7SRHOBH \
| 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: 0a8d2437fddaa2ef8d79bdb3f944ee09c97d1727526b77b193f5b6e07460ff5b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "139ec402ad0e1eb9a222ba5de5aabe52d4f4ecb4b17652c11a36353f772a498d",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-08-25T20:00:08Z",
"title_canon_sha256": "d9b9e374d9c62575e2ec51bdf3a3e031b5b52bc415a7a657f30571db04e94c86"
},
"schema_version": "1.0",
"source": {
"id": "1008.4359",
"kind": "arxiv",
"version": 4
}
}