Pith Number
pith:YDOAM4Y5
pith:2026:YDOAM4Y53WD2OUQBCLE7VXEUYF
not attested
not anchored
not stored
refs pending
The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos
arxiv:2606.19443 v1 · 2026-06-17 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YDOAM4Y53WD2OUQBCLE7VXEUYF}
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
✓
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 | 2026-06-19T16:12:25.792472Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c0dc06731ddd87a7520112c9fadc94c15b2429f9524e4e0b6e2c6ea202a793a3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YDOAM4Y53WD2OUQBCLE7VXEUYF \
| 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: c0dc06731ddd87a7520112c9fadc94c15b2429f9524e4e0b6e2c6ea202a793a3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0544a5cd6b36bfd7cfc3d85ef97b9aa9fc3c018af19d9cc8c81b244886609735",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2026-06-17T18:00:04Z",
"title_canon_sha256": "dd77c1f372b05e600b989729442b6d5a63e41d8693e985f9a3e0ab57c3734fc1"
},
"schema_version": "1.0",
"source": {
"id": "2606.19443",
"kind": "arxiv",
"version": 1
}
}