Pith. sign in

REVIEW 1 cited by

The Low-Spin Black Hole in LMC X-3

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1402.0148 v1 pith:YAYAAJPX submitted 2014-02-02 astro-ph.HE

classification astro-ph.HE
keywords spinblackholex-rayspectraaccountbinarybuilding
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Building upon a new dynamical model for the X-ray binary LMC X-3, we measure the spin of its black hole primary via the continuum-fitting method. We consider over one thousand thermal-state RXTE X-ray spectra of LMC X-3. Using a large subset of these spectra, we constrain the spin parameter of the black hole to be spin = 0.21(+0.18,-0.22), 90% confidence. Our estimate of the uncertainty in spin takes into account a wide range of systematic errors. We discuss evidence for a correlation between a black hole's spin and the complexity of its X-ray spectrum.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Astronomical X-ray Polarimetry as a diagnostic for questions of fundamental Physics. What we learned from the Imaging X-Ray Polarimetry Explorer (IXPE)

    astro-ph.IM 2024-12 unverdicted

    A conference review of IXPE's first three years concludes that X-ray polarimetry is a promising new diagnostic for fundamental physics, with the most promising target being axion-like particle induced polarization in ...

Pith tools