Pith Number
pith:RW2WDLPI
pith:2012:RW2WDLPIGJXG6XSWRHLCMD2BBZ
not attested
not anchored
not stored
refs pending
Origin of Two Types of X-Ray Outbursts in Be/X-Ray Binaries. I. Accretion Scenarios
arxiv:1211.5225 v1 · 2012-11-22 · astro-ph.HE · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RW2WDLPIGJXG6XSWRHLCMD2BBZ}
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 | 2026-05-18T01:53:01.624539Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8db561ade8326e6f5e5689d6260f410e6a248f33449f9bc9171c42903199776e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RW2WDLPIGJXG6XSWRHLCMD2BBZ \
| 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: 8db561ade8326e6f5e5689d6260f410e6a248f33449f9bc9171c42903199776e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "532d17b26518f3b800f800abe35f72532fbc7578ed90c42d682c36294f0baa90",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2012-11-22T08:22:27Z",
"title_canon_sha256": "dba0f07fe671435a02210bb3628619a1830d384e9abe8b200646a87c7edc5f88"
},
"schema_version": "1.0",
"source": {
"id": "1211.5225",
"kind": "arxiv",
"version": 1
}
}