Pith Number
pith:JXF2UNBT
pith:1997:JXF2UNBTDHK4Z6KVP5N5AD6RWA
not attested
not anchored
not stored
refs pending
Pulsations in red supergiants with high L/M ratio -- Implications for the stellar and circumstellar structure of supernova progenitors
arxiv:astro-ph/9705097 v1 · 1997-05-13 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{JXF2UNBTDHK4Z6KVP5N5AD6RWA}
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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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:07:38.344920Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4dcbaa343319d5ccf9557f5bd00fd1b03f912d920126114a12db6ad645727bc9
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/JXF2UNBTDHK4Z6KVP5N5AD6RWA \
| 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: 4dcbaa343319d5ccf9557f5bd00fd1b03f912d920126114a12db6ad645727bc9
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3128f558fa7def78560f9dfc02c5ccf791a71b3db0d8d1a5d1f310d175f5682f",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1997-05-13T16:21:50Z",
"title_canon_sha256": "90c18f4166bc20063fea60ae68a52c9dd42599921acfdb8f7aac181ac9e8e08b"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9705097",
"kind": "arxiv",
"version": 1
}
}