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This article gives a very brief introduction about measuring the mass andradius of neutron star from X-ray observations. The masses and radii of neutronstars can be determined from photospheric radius expansion bursts in low-massX-ray binaries, X-ray pulse profile modeling in accreting X-ray pulsars,gravitational redshift measurement in low-mass X-ray binaries and thermal X-rayspectral fitting in quiescent low-mass X-ray binaries.

Constraints on the mass and radius of neutron stars from X-ray observations