Pith Number
pith:Y2SRHBGQ
pith:2010:Y2SRHBGQ2M3ND6BXK7D35WC4RF
not attested
not anchored
not stored
refs pending
A near-infrared morphological comparison of high-redshift submm and radio galaxies: massive star-forming discs vs relaxed spheroids
arxiv:1005.5176 v2 · 2010-05-27 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{Y2SRHBGQ2M3ND6BXK7D35WC4RF}
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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4
Citations
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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 | 2026-05-18T02:07:07.048653Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c6a51384d0d336d1f83757c7bed85c8970e2929af1c2add2113c5d729b0507ff
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Y2SRHBGQ2M3ND6BXK7D35WC4RF \
| 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: c6a51384d0d336d1f83757c7bed85c8970e2929af1c2add2113c5d729b0507ff
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0ee504af868a2d20c0c2397261b3476720150d2be4710f813b287ec1ed8ed804",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-05-27T20:46:50Z",
"title_canon_sha256": "9dc9550c557f3e58f29aa84e7ba93b2870eac74de0156c04038ab84f8c9971b7"
},
"schema_version": "1.0",
"source": {
"id": "1005.5176",
"kind": "arxiv",
"version": 2
}
}