Pith Number
pith:C3WQ3HAV
pith:2016:C3WQ3HAVT4HXHGJHULANQSVDNZ
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refs pending
The prospects of measuring the angular power spectrum of the diffuse Galactic synchrotron emission with SKA1 Low
arxiv:1610.08184 v2 · 2016-10-26 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{C3WQ3HAVT4HXHGJHULANQSVDNZ}
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Record completeness
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Bitcoin timestamp
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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 | 2026-05-18T00:39:39.829024Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
16ed0d9c159f0f739927a2c0d84aa36e5e8b197c6e3ab658ada8e36a9f4c7a2c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/C3WQ3HAVT4HXHGJHULANQSVDNZ \
| 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: 16ed0d9c159f0f739927a2c0d84aa36e5e8b197c6e3ab658ada8e36a9f4c7a2c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dd119625acede44a7192669e7dc924f61ed598774b66c8f193bee86a943bead3",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2016-10-26T05:48:52Z",
"title_canon_sha256": "f6d554291df433885957b1a5c2ddf8dcb6fe9f46085668e2e58167fc5f73eb39"
},
"schema_version": "1.0",
"source": {
"id": "1610.08184",
"kind": "arxiv",
"version": 2
}
}