Pith Number
pith:H4VUGZKK
pith:2009:H4VUGZKKEBXCUTFZDDMMJRMRY3
not attested
not anchored
not stored
refs pending
Impact of helium diffusion and helium-flash-induced carbon production on gravity-mode pulsations in subdwarf B stars
arxiv:0910.5641 v1 · 2009-10-29 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{H4VUGZKKEBXCUTFZDDMMJRMRY3}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T02:11:01.737979Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3f2b43654a206e2a4cb918d8c4c591c6e85446c4c796826a6a1f7ace338f6b18
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/H4VUGZKKEBXCUTFZDDMMJRMRY3 \
| 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: 3f2b43654a206e2a4cb918d8c4c591c6e85446c4c796826a6a1f7ace338f6b18
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e61fb0031dbd71e074a55c0acfb2cb370c5af6bbca5f7e8b4947bebd525f699a",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2009-10-29T13:49:25Z",
"title_canon_sha256": "5c44c303f5a1b85bac3a1bc9a7a9ad94326ca90a9372ddb3026b879414d25d52"
},
"schema_version": "1.0",
"source": {
"id": "0910.5641",
"kind": "arxiv",
"version": 1
}
}