Pith Number
pith:XBEVZ4N2
pith:2017:XBEVZ4N26IO7ZDS4URCBKW327L
not attested
not anchored
not stored
refs pending
Can the observed E/B ratio for dust galactic foreground be explained by sub-Alfvenic turbulence?
arxiv:1707.06276 v2 · 2017-07-19 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XBEVZ4N26IO7ZDS4URCBKW327L}
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 | 2026-05-18T00:36:38.226587Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b8495cf1baf21dfc8e5ca444155b7afad04deee17e062e84bc775e2580991bf0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XBEVZ4N26IO7ZDS4URCBKW327L \
| 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: b8495cf1baf21dfc8e5ca444155b7afad04deee17e062e84bc775e2580991bf0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "91a8e18b91bdacd912178e492a8748a83c95cee2244dd27b84a389e503d376ad",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-07-19T19:59:59Z",
"title_canon_sha256": "be8f462b7fbdbbf210ca5f82283938f6ed3da9372c4137a8785256e6953e548c"
},
"schema_version": "1.0",
"source": {
"id": "1707.06276",
"kind": "arxiv",
"version": 2
}
}