Pith Number
pith:WFFGI5EY
pith:2013:WFFGI5EYI7NT5GHMYBDCEYJLRL
not attested
not anchored
not stored
refs pending
How cosmic-ray electron propagation affects radio-far-infrared correlations in M31 and M33
arxiv:1307.7991 v1 · 2013-07-30 · astro-ph.GA · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WFFGI5EYI7NT5GHMYBDCEYJLRL}
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 | 2026-05-18T01:48:32.859079Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b14a64749847db3e98ecc04622612b8aea8df86ed64e38f9e513efb4b437d2ba
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WFFGI5EYI7NT5GHMYBDCEYJLRL \
| 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: b14a64749847db3e98ecc04622612b8aea8df86ed64e38f9e513efb4b437d2ba
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d2884bec3c1ccef8c5ab7e42da8ebc62d053e1a395036833f7e171d024314a86",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2013-07-30T14:16:50Z",
"title_canon_sha256": "7626f2acf68c40f739f25616488fc36aa67c94bf77225cacd3ab1bacbde25f7e"
},
"schema_version": "1.0",
"source": {
"id": "1307.7991",
"kind": "arxiv",
"version": 1
}
}