Pith Number
pith:WEMM3JKN
pith:2017:WEMM3JKN5XZ3LL7FA72FQY6KW4
not attested
not anchored
not stored
refs pending
On the Optical-to-Silicate Extinction Ratio as a Probe of the Dust Size in Active Galactic Nuclei
arxiv:1704.01103 v1 · 2017-04-04 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WEMM3JKN5XZ3LL7FA72FQY6KW4}
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 | 2026-05-18T00:44:51.207207Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b118cda54dedf3b5afe507f45863cab7116a14be8b6ad0dc19be19f62f0f1f5a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WEMM3JKN5XZ3LL7FA72FQY6KW4 \
| 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: b118cda54dedf3b5afe507f45863cab7116a14be8b6ad0dc19be19f62f0f1f5a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "88107c5f7d3b8da0278843400b6ee27ce2471806c89e99636462a6c08625fc68",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-04-04T16:47:54Z",
"title_canon_sha256": "204932aeef73db2bcca7e970b9998efeb99b0768b4b50ef1707e3bb51907347a"
},
"schema_version": "1.0",
"source": {
"id": "1704.01103",
"kind": "arxiv",
"version": 1
}
}