Pith Number
pith:IQ6R6QWJ
pith:2016:IQ6R6QWJ5L23NF4KRZC2HAQBGT
not attested
not anchored
not stored
refs pending
Using the outskirts of galaxy clusters to determine their mass accretion rate
arxiv:1612.03909 v2 · 2016-12-12 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IQ6R6QWJ5L23NF4KRZC2HAQBGT}
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 | 2026-05-18T00:54:26.020427Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
443d1f42c9eaf5b6978a8e45a3820134e64fa43d8fd82e3e84d9eaf8018188c2
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IQ6R6QWJ5L23NF4KRZC2HAQBGT \
| 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: 443d1f42c9eaf5b6978a8e45a3820134e64fa43d8fd82e3e84d9eaf8018188c2
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "288b7b3eb27a2ad71f1e0b4eebb2769a3a953f7d34028ed7bffbb067ca1d2725",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2016-12-12T21:00:01Z",
"title_canon_sha256": "71fad30292353a144af7678e2babd411a171a9c67ce9ac1e2b9cb4cc9956c114"
},
"schema_version": "1.0",
"source": {
"id": "1612.03909",
"kind": "arxiv",
"version": 2
}
}