Sourcejournal articleno stored text

Constraining the properties of the thermonuclear burst oscillation source XTE J1814−338 through pulse profile modelling

Yves Kini, Tuomo Salmi, Serena Vinciguerra, Anna L Watts, Anna Bilous, Duncan K Galloway, Emma van der Wateren, Guru Partap Khalsa, Slavko Bogdanov, Johannes Buchner, Valery SuleimanovMonthly Notices of the Royal Astronomical SocietyPublished Oct 21, 2024doi 10.1093/mnras/stae2398 Original︎ ↗Archived copy

Claims2

ExaminationsNone

TextNot stored

VersionsOne known

CopiesNone recorded

CorrectionsNone recorded

Facts checked Nov 11, 2026

ReachNo copies recorded

StructureIn 2 claims' maps0 sources downstream across 2 claims

EvidenceNot yet read

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.

As quoted

we infer XTE J1814–338 to be located at a distance of 7.2+0.3−0.4 kpc, with a mass of 1.21+0.05−0.05 M⊙

The pulsar XTE J1814-338 has an inferred radius of about 7 km, smaller than neutron star models predictVerified

Not yet read by this claim’s Steward.

As quoted

Our analysis yielded the following results for XTE J1814–338: a mass of $1.21^{+0.05}_{-0.05}~M_{\odot}$, a radius of $7.0^{+0.4}_{-0.4}~km$, and a distance of $7.2^{+0.3}_{-0.4}~kpc$.

Pulse profile modeling of XTE J1814-338's thermonuclear burst oscillations yields a radius near 7 km and a mass near 1.2 solar massesVerified

Not yet read by this claim’s Steward.

Lineage across 2 claims

Draws on · none recorded

This source

Constraining the properties of the thermonuclear burst oscillation source XTE J1814−338 t…

in 2 claims' maps

Drawn on by · none recorded

Record

Kind: journal article
Authors: Yves Kini, Tuomo Salmi, Serena Vinciguerra, Anna L Watts, Anna Bilous, Duncan K Galloway, Emma van der Wateren, Guru Partap Khalsa, Slavko Bogdanov, Johannes Buchner, Valery Suleimanov
Publisher: Monthly Notices of the Royal Astronomical Society
Published: Oct 21, 2024
DOI: 10.1093/mnras/stae2398
Link: https://arxiv.org/abs/2405.10717
Archived copy: https://web.archive.org/web/20260901161827/https://arxiv.org/abs/2405.10717
Stored text: None; quoted passages only
Claims extracted: Not recorded
Versions: One known
Copies: None recorded
Corrections: None recorded
Facts checked: Nov 11, 2026

History 1

Aug 5, 2026Entered the graphEntered the graph; no copy stored