Pith Number
pith:XPIKBKKJ
pith:2020:XPIKBKKJYSMVVUFNZVM3KJMYBK
not attested
not anchored
not stored
refs pending
Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
arxiv:2012.08629 v2 · 2020-12-15 · astro-ph.CO · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XPIKBKKJYSMVVUFNZVM3KJMYBK}
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
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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 | 2026-07-05T02:52:59.393150Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
bbd0a0a949c4995ad0adcd59b525980aa48c620b237269b61bc5296d71ec5482
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XPIKBKKJYSMVVUFNZVM3KJMYBK \
| 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: bbd0a0a949c4995ad0adcd59b525980aa48c620b237269b61bc5296d71ec5482
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "ce5066b974b5caf66ff116cf71163db0db5c8fa770869a168a64192e77a5878f",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2020-12-15T21:39:34Z",
"title_canon_sha256": "6ea5c9275d4746881619b24357d4e26ec23fa727ab4ce6523d4668cd62be2b7d"
},
"schema_version": "1.0",
"source": {
"id": "2012.08629",
"kind": "arxiv",
"version": 2
}
}