Pith Number
pith:XQP73Z2E
pith:2018:XQP73Z2EDDPK6GADT6YATTEJVC
not attested
not anchored
not stored
refs pending
Evidence of Hubble flow-like motion of young stellar populations away from the Perseus arm
arxiv:1812.11102 v1 · 2018-12-28 · astro-ph.GA · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XQP73Z2EDDPK6GADT6YATTEJVC}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
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 | 2026-05-17T23:55:18.707634Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
bc1ffde74418deaf18039fb009cc89a89da1df5a16a4d64c5ba1e2a1abecbfc1
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XQP73Z2EDDPK6GADT6YATTEJVC \
| 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: bc1ffde74418deaf18039fb009cc89a89da1df5a16a4d64c5ba1e2a1abecbfc1
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2c5189198a5080c41584f602521afda5653af1f47f10528a57c6026b0e50166d",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2018-12-28T16:35:27Z",
"title_canon_sha256": "fc22b20f91c937a26bf126f19734d23b4b040bbab2033c8b21ab7e6abac6d6dc"
},
"schema_version": "1.0",
"source": {
"id": "1812.11102",
"kind": "arxiv",
"version": 1
}
}