The National Spherical Torus Experiment ͑NSTX͒ routinely studies overdense plasmas with n e of ͑1-5͒ ϫ 10 19 m −3 and total magnetic field of Ͻ0.6 T, so that the first several electron cyclotron harmonics are overdense. The electrostatic electron Bernstein wave ͑EBW͒ can propagate in overdense plasmas, exhibits strong absorption, and is thermally emitted at electron cyclotron harmonics. These properties allow thermal EBW emission to be used for local T e measurement. A significant upgrade to the previous NSTX EBW emission diagnostic to measure thermal EBW emission via the oblique B-X-O mode conversion process has been completed. The new EBW diagnostic consists of two remotely steerable, quad-ridged horn antennas, each of which is coupled to a dual channel radiometer. Fundamental ͑8-18 GHz͒ and second and third harmonic ͑18-40 GHz͒ thermal EBW emission and polarization measurements can be obtained simultaneously.