Pith Number
pith:HKBMMG3X
pith:2014:HKBMMG3X5H4JRPDVJI62ENYDYG
not attested
not anchored
not stored
refs pending
The physical nature of the cosmic accretion of baryons and dark matter into halos and their galaxies
arxiv:1412.0662 v2 · 2014-12-01 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HKBMMG3X5H4JRPDVJI62ENYDYG}
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 | 2026-05-18T01:35:49.642961Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3a82c61b77e9f898bc754a3da23703c1af6c31ab0b9f51f06e50f514fa9621f8
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HKBMMG3X5H4JRPDVJI62ENYDYG \
| 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: 3a82c61b77e9f898bc754a3da23703c1af6c31ab0b9f51f06e50f514fa9621f8
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "ef22dee7428fa775e0bd9a0a030b163feefaf4805b02eef30c94cbea8b415f5a",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2014-12-01T21:00:07Z",
"title_canon_sha256": "7248aa667f28a104aac464965c7bd5f642f13db3a2ebc7d239b095305a395394"
},
"schema_version": "1.0",
"source": {
"id": "1412.0662",
"kind": "arxiv",
"version": 2
}
}