https://arxiv.org/abs/2506.10032
Author not recordedDate not recordedOriginal︎ ↗Archived copy
Examinations
None recorded. An examination is commissioned by a claim’s Steward for what its claim rests on; a review of the document for its own sake is asked for as a request bearing on it.
Text
No stored copy. Only the passages claims quote are recorded.
resulted in mass (M) and radius (R) parameters of (R/km, M/M⊙) = (7.0+0.4−0.4, 1.21+0.05−0.05) ... the extraordinarily small radius poses a problem for establishing a proper neutron star model
Not yet read by this claim’s Steward.
The pulse-profile modeling of the accretion-powered millisecond pulsar XTE J1814-338 by a single uniform-temperature hot-spot resulted in mass (M) and radius (R) parameters of $(R/\text{km}, M/M_{\odot}) = (7.0^{+0.4}_{-0.4}, 1.21^{+0.05}_{-0.05})$ [1].
Not yet read by this claim’s Steward.
Lineage across 2 claims
Record
- Kind
- unknown
- Authors
- Not recorded
- Publisher
- Not recorded
- Published
- Not recorded
- DOI
- None
- Link
- https://arxiv.org/abs/2506.10032
- Archived copy
- https://web.archive.org/web/20250810220410/https://arxiv.org/abs/2506.10032
- Stored text
- None; quoted passages only
- Claims extracted
- Not recorded
- Versions
- One known
- Copies
- None recorded
- Corrections
- None recorded
- Facts checked
- Nov 9, 2026
History 2
- Nov 9, 2026FactsFacts fetcher · Facts looked up
- Aug 5, 2026Entered the graphEntered the graph; no copy stored