Pith Number
pith:QQSPVGQX
pith:2016:QQSPVGQXWH24TJHRUNZNVG63WI
not attested
not anchored
not stored
refs pending
The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s
arxiv:1605.01058 v1 · 2016-05-03 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{QQSPVGQXWH24TJHRUNZNVG63WI}
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 | 2026-05-18T01:13:47.200702Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8424fa9a17b1f5c9a4f1a372da9bdbb235bc37989d0e2c5d2c91fb99f44b246d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/QQSPVGQXWH24TJHRUNZNVG63WI \
| 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: 8424fa9a17b1f5c9a4f1a372da9bdbb235bc37989d0e2c5d2c91fb99f44b246d
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "29405642aa2b7ac70162f9dd3912ac1d546321f3c83e05c62aefd4f3d28e912d",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2016-05-03T20:00:01Z",
"title_canon_sha256": "214cba40807036ab1d331450f9b2499f61db92133e3e5c8a171874193be8883b"
},
"schema_version": "1.0",
"source": {
"id": "1605.01058",
"kind": "arxiv",
"version": 1
}
}