Pith Number
pith:BCQNAEWR
pith:2016:BCQNAEWRARE6CWUP5XJKZ5HY3O
not attested
not anchored
not stored
refs pending
Magnetic flux density from the relative circular motion of stars and partially ionized gas in the Galaxy mid-plane vicinity
arxiv:1610.07544 v1 · 2016-10-24 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BCQNAEWRARE6CWUP5XJKZ5HY3O}
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 | 2026-05-18T00:54:28.221515Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
08a0d012d10449e15a8fedd2acf4f8db8c46efffc4d6e5d90de20ee50fc7fdcd
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BCQNAEWRARE6CWUP5XJKZ5HY3O \
| 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: 08a0d012d10449e15a8fedd2acf4f8db8c46efffc4d6e5d90de20ee50fc7fdcd
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d905df2596f99ace87c170791e1884150de5ac60b65671a94bd3e5b5bd93a4ad",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2016-10-24T18:54:46Z",
"title_canon_sha256": "7ee6e7e7085ab7d05adb32f045000784a3ebe833845e4866cfd087fc72b596ac"
},
"schema_version": "1.0",
"source": {
"id": "1610.07544",
"kind": "arxiv",
"version": 1
}
}