Pith Number
pith:KGPTJNMS
pith:2002:KGPTJNMSZ5BSAZQNLKYX4JVIJH
not attested
not anchored
not stored
refs pending
Slow relative motion of IRAS galaxies at small separations: implications for galaxy formation models
arxiv:astro-ph/0201145 v1 · 2002-01-10 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KGPTJNMSZ5BSAZQNLKYX4JVIJH}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-07-04T14:11:45.258248Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
519f34b592cf4320660d5ab17e26a849d5bfc555bc52903c11f6d3d450c6c6b5
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KGPTJNMSZ5BSAZQNLKYX4JVIJH \
| 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: 519f34b592cf4320660d5ab17e26a849d5bfc555bc52903c11f6d3d450c6c6b5
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5c050e9d6f965aa6f99a9ea43078f0c07914f616bdf8bf07d14dc767447735e3",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2002-01-10T01:55:54Z",
"title_canon_sha256": "7aa5c4c21e097ced332404b6ba4c78fd605e271ebddce87eb7929a0ce5441cf4"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0201145",
"kind": "arxiv",
"version": 1
}
}