Pith Number
pith:SQA2EKDR
pith:2016:SQA2EKDRFVB5XVPXRG3T5RYU3R
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refs pending
On the Relation between the Mysterious 21 Micrometer Emission Feature of Post-Asymptotic Giant Branch Stars and Their Mass Loss Rates
arxiv:1605.03166 v1 · 2016-05-10 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{SQA2EKDRFVB5XVPXRG3T5RYU3R}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
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4
Citations
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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 | 2026-05-18T01:11:30.655760Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
9401a228712d43dbd5f789b73ec714dc7e348e4fd74aaa2e60608e06ea430ea0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/SQA2EKDRFVB5XVPXRG3T5RYU3R \
| 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: 9401a228712d43dbd5f789b73ec714dc7e348e4fd74aaa2e60608e06ea430ea0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e5d0a76bdbe0be05f5b5b2154b1863e6b7f3a92fafb5710f62cfa309af7cd109",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2016-05-10T19:43:03Z",
"title_canon_sha256": "603ffdabfceb3a7b6c7ef81442faaeb4ebf65ed9da0a0b5c7974579e677692f2"
},
"schema_version": "1.0",
"source": {
"id": "1605.03166",
"kind": "arxiv",
"version": 1
}
}