Pith Number
pith:TKBYUOUI
pith:2010:TKBYUOUIMYV2PHC4XX347XU5UY
not attested
not anchored
not stored
refs pending
The Abundance Pattern of O, Ne, Mg, and Fe in the Interstellar Medium of S0 Galaxy NGC 4382 Observed with Suzaku
arxiv:1004.2960 v1 · 2010-04-17 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{TKBYUOUIMYV2PHC4XX347XU5UY}
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 | 2026-05-18T02:07:57.232110Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
9a838a3a88662ba79c5cbdf7cfde9da62ffdaa699ef964c183d309a05833ad35
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/TKBYUOUIMYV2PHC4XX347XU5UY \
| 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: 9a838a3a88662ba79c5cbdf7cfde9da62ffdaa699ef964c183d309a05833ad35
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "66437cea8dfcc3c38925c8ee8409f1d999d9602ae4a1845693a13a6deb9ca5ea",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-04-17T14:29:47Z",
"title_canon_sha256": "7f15dc985b2c7d085a127277e8026d0a2e772c14ff74e2ba564a602e4c59f0d1"
},
"schema_version": "1.0",
"source": {
"id": "1004.2960",
"kind": "arxiv",
"version": 1
}
}