Pith Number
pith:4RBPYQLP
pith:2015:4RBPYQLPGTD5NU3LCBD5TE6VBF
not attested
not anchored
not stored
refs pending
The mass accretion rate of galaxy clusters: a measurable quantity
arxiv:1501.01977 v4 · 2015-01-08 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4RBPYQLPGTD5NU3LCBD5TE6VBF}
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 | 2026-05-18T01:18:54.454627Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e442fc416f34c7d6d36b1047d993d5095ed702e18eed20b074d6811fa1652ad3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4RBPYQLPGTD5NU3LCBD5TE6VBF \
| 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: e442fc416f34c7d6d36b1047d993d5095ed702e18eed20b074d6811fa1652ad3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "afc027d2f77f3867c27ae34b2691fbaae16941be6d65f874039e8993b8e238a0",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2015-01-08T21:00:33Z",
"title_canon_sha256": "71b63582a4ae7e8ed942c747df92dca728d1657deb23451d8fd7e5285ae102fd"
},
"schema_version": "1.0",
"source": {
"id": "1501.01977",
"kind": "arxiv",
"version": 4
}
}