Pith Number
pith:I3TFG32T
pith:2017:I3TFG32TEKFV66IFG6UQDPR7JY
not attested
not anchored
not stored
refs pending
Strong lensing modeling in galaxy clusters as a promising method to test cosmography I. Parametric dark energy models
arxiv:1711.00829 v2 · 2017-11-02 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{I3TFG32TEKFV66IFG6UQDPR7JY}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T00:03:49.934723Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
46e6536f53228b5f790537a901be3f4e01c12ef5ebdf3f1a42ec6c346ad8ab55
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/I3TFG32TEKFV66IFG6UQDPR7JY \
| 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: 46e6536f53228b5f790537a901be3f4e01c12ef5ebdf3f1a42ec6c346ad8ab55
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "734dc9eaace4d1354df9563759c70eea65334d3b8b143c6c06be2b5ed9c246ba",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2017-11-02T17:24:20Z",
"title_canon_sha256": "3229c5f73e81a513815b5c2f535dcdfcc62c1be49d771dfae65e31164cf1fa98"
},
"schema_version": "1.0",
"source": {
"id": "1711.00829",
"kind": "arxiv",
"version": 2
}
}