Pith Number
pith:2XWTSVI3
pith:2024:2XWTSVI3Z34HLE7VZDQ4XXRED5
not attested
not anchored
not stored
refs pending
Do Neutron Star Ultra-Luminous X-Ray Sources Masquerade as Intermediate Mass Black Holes in Radio and X-Ray?
arxiv:2410.23335 v1 · 2024-10-30 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{2XWTSVI3Z34HLE7VZDQ4XXRED5}
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
✓
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 | 2026-07-05T09:28:58.607142Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d5ed39551bcef87593f5c8e1cbde241f5c218e4b7a2e854d36c6c7e6ed421f01
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2XWTSVI3Z34HLE7VZDQ4XXRED5 \
| 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: d5ed39551bcef87593f5c8e1cbde241f5c218e4b7a2e854d36c6c7e6ed421f01
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "b476467ec5cc1a33315ab6e5efc3ab52d4f9700d3f54a3ffd2429fd0c7f7305c",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2024-10-30T18:00:00Z",
"title_canon_sha256": "c99b5a26abb1e6f2d698fb9cfcf09ef4a5a4e91b500fa8bab674bf1b754dcb6d"
},
"schema_version": "1.0",
"source": {
"id": "2410.23335",
"kind": "arxiv",
"version": 1
}
}