Pith Number
pith:QTMRKGFE
pith:2019:QTMRKGFET3DI3ZKCZ7HZRTDNMI
not attested
not anchored
not stored
refs pending
Do Galaxy Morphologies Really Affect the Efficiency of Star Formation during the Phase of Galaxy Transition?
arxiv:1903.03505 v1 · 2019-03-08 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{QTMRKGFET3DI3ZKCZ7HZRTDNMI}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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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 | 2026-05-17T23:49:01.611379Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
84d91518a49ec68de542cfcf98cc6d622a9aec5812d5bfd350d212472b0d539e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/QTMRKGFET3DI3ZKCZ7HZRTDNMI \
| 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: 84d91518a49ec68de542cfcf98cc6d622a9aec5812d5bfd350d212472b0d539e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "c642e491d2a8f00533fb6f05c8e91eb937e45fd7af18ced378d9ac3f69d5f721",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2019-03-08T15:32:19Z",
"title_canon_sha256": "d7f8a84ce8853d5f8f6b7ab2b8c79d7e006b6e0c55a7101d3286b34c7c6d8fd0"
},
"schema_version": "1.0",
"source": {
"id": "1903.03505",
"kind": "arxiv",
"version": 1
}
}