SIMBAD references

We report on a simultaneous NuSTAR and Swift observation of the neutron star low-mass X-ray binary 4U 1728-34. We identified and removed four Type I X-ray bursts during the observation in order to study the persistent emission. The continuum spectrum is hard and described well by a blackbody with kT=1.5 keV and a cutoff power law with Γ=1.5, and a cutoff temperature of 25 keV. Residuals between 6 and 8 keV provide strong evidence of a broad Fe Kα line. By modeling the spectrum with a relativistically blurred reflection model, we find an upper limit for the inner disk radius of {R}_{∈}\leqslant 2{R}_{ISCO}. Consequently, we find that R_NS <= 23 km, assuming M=1.4 M_☉ and a=0.15. We also find an upper limit on the magnetic field of B <= 2 x 10^8 G.