Pith Number
pith:PGJDHMTU
pith:2014:PGJDHMTUSYMH3H6EBOYKSLLIRP
not attested
not anchored
not stored
refs pending
Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?
arxiv:1410.7723 v3 · 2014-10-28 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{PGJDHMTUSYMH3H6EBOYKSLLIRP}
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 | 2026-05-18T02:20:09.922363Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
799233b27496187d9fc40bb0a92d688bc7b68807cf3522a7d3f61d87b22ead7c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/PGJDHMTUSYMH3H6EBOYKSLLIRP \
| 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: 799233b27496187d9fc40bb0a92d688bc7b68807cf3522a7d3f61d87b22ead7c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "1fe5c0eb5ac7f550e47692e6c54d4294a2b3e727475cfa22d2736f2ca9785a04",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-10-28T18:23:59Z",
"title_canon_sha256": "3ab6054f554a143d12102639c13f0cb385843382eefbe3879d1ed7700f2231d7"
},
"schema_version": "1.0",
"source": {
"id": "1410.7723",
"kind": "arxiv",
"version": 3
}
}