Pith Number
pith:XWC4FIIH
pith:2019:XWC4FIIHHQ2AIILHO3CH5CGFRV
not attested
not anchored
not stored
refs pending
The Richness-to-Mass Relation of CAMIRA Galaxy Clusters from Weak-lensing Magnification in the Subaru Hyper Suprime-Cam Survey
arxiv:1909.02042 v2 · 2019-09-04 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XWC4FIIHHQ2AIILHO3CH5CGFRV}
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 | 2026-07-05T01:00:13.703656Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
bd85c2a1073c3404216776c47e88c58d7423d60b0abbac73e8c351a753fff201
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XWC4FIIHHQ2AIILHO3CH5CGFRV \
| 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: bd85c2a1073c3404216776c47e88c58d7423d60b0abbac73e8c351a753fff201
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "86ee9c349a6fe43fb23a840a95210f1064bc1f20ad80dd4c6e700d445e20f3b1",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2019-09-04T18:34:32Z",
"title_canon_sha256": "6c8baa7904c2b78e1fe2e5ee6f28bc9216bb9d682e803f7385aaacea54db255f"
},
"schema_version": "1.0",
"source": {
"id": "1909.02042",
"kind": "arxiv",
"version": 2
}
}