Pith Number
pith:Z3PBMCWB
pith:2007:Z3PBMCWBCN2KJX6VGQ7LQUXCTR
not attested
not anchored
not stored
refs pending
The Detection of Far Ultraviolet Line Emission from Balmer-Dominated Supernova Remnants in the Large Magellanic Cloud
arxiv:astro-ph/0703809 v1 · 2007-03-30 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{Z3PBMCWBCN2KJX6VGQ7LQUXCTR}
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 | 2026-05-18T02:40:24.816369Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
cede160ac11374a4dfd5343eb852e29c59ffee17bf2669278386b4ef28c51a23
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Z3PBMCWBCN2KJX6VGQ7LQUXCTR \
| 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: cede160ac11374a4dfd5343eb852e29c59ffee17bf2669278386b4ef28c51a23
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2b5d6b6ab68e54c290000729b565dc4d27f4945bca95af78a2e14bc0a55792e1",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2007-03-30T19:57:19Z",
"title_canon_sha256": "69dd118fbd78c5e3b8687221ef83fae4156946382b06a6ab9ff09da221bbb3cb"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0703809",
"kind": "arxiv",
"version": 1
}
}