Pith Number
pith:CTMJL27A
pith:2012:CTMJL27ACL3P2T326O4OCZ2JMM
not attested
not anchored
not stored
refs pending
Scenarios to explain extreme Be depletion in solar-like stars: accretion or rotation effects ?
arxiv:1209.1812 v1 · 2012-09-09 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{CTMJL27ACL3P2T326O4OCZ2JMM}
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 | 2026-05-18T01:54:38.092105Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
14d895ebe012f6fd4f7af3b8e167496326d6e12aa4edf4cc5124b5ac62b89bc0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CTMJL27ACL3P2T326O4OCZ2JMM \
| 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: 14d895ebe012f6fd4f7af3b8e167496326d6e12aa4edf4cc5124b5ac62b89bc0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e98bae86ebb14bfaf321ee266ae77a96cfa2f034a6b7ceb0478901bf9d1ceaf8",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2012-09-09T16:44:25Z",
"title_canon_sha256": "e1d1efe70e9a1efab6859af6620083b0cb903f063e911beada66f8d049fb3128"
},
"schema_version": "1.0",
"source": {
"id": "1209.1812",
"kind": "arxiv",
"version": 1
}
}