Pith Number
pith:ZJYOA63R
pith:2016:ZJYOA63RJUGLFWBFQJJQ222BMO
not attested
not anchored
not stored
refs pending
How similar is the stellar structure of low-mass late-type galaxies to that of early-type dwarfs?
arxiv:1605.06189 v2 · 2016-05-20 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{ZJYOA63RJUGLFWBFQJJQ222BMO}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:11:10.253046Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ca70e07b714d0cb2d82582530d6b4163be462ebf1ded8f6e9a5acdc29fd1ec3a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/ZJYOA63RJUGLFWBFQJJQ222BMO \
| 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: ca70e07b714d0cb2d82582530d6b4163be462ebf1ded8f6e9a5acdc29fd1ec3a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f8e06faa6c0b9a682cc51c210045aba826feb49295ae36d43d63cfdcf282b0e2",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2016-05-20T01:09:52Z",
"title_canon_sha256": "48de25859410d8677000151cb6c1888064050a5c57870e9037720cc035cd64ca"
},
"schema_version": "1.0",
"source": {
"id": "1605.06189",
"kind": "arxiv",
"version": 2
}
}