Pith Number
pith:KEDNWFTT
pith:2025:KEDNWFTT2TN2AIHGXH2W7N5I7C
not attested
not anchored
not stored
refs pending
Unified weak lensing constraints on the evolution of the mass -- X-ray luminosity relation for galaxy clusters
arxiv:2505.21659 v1 · 2025-05-27 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KEDNWFTT2TN2AIHGXH2W7N5I7C}
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
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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.
Cited by
Receipt and verification
| First computed | 2026-07-05T11:11:01.659559Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5106db1673d4dba020e6b9f56fb7a8f8876356b881eb1a17e749b18f5b4db2c3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KEDNWFTT2TN2AIHGXH2W7N5I7C \
| 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: 5106db1673d4dba020e6b9f56fb7a8f8876356b881eb1a17e749b18f5b4db2c3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a86878ac3a44c9a33a9389c60468a17cac81d1dd0edc019932fbfe4b015b076c",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2025-05-27T18:34:38Z",
"title_canon_sha256": "a33ba6310f2db5f4f2346002e44d6c29bcccf53e6c9ad793bfd19056e6ca95e2"
},
"schema_version": "1.0",
"source": {
"id": "2505.21659",
"kind": "arxiv",
"version": 1
}
}