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We present an update of the grid of detailed atmosphere models andhomogeneous synthetic spectra for hot, high-gravity subdwarf stars.High-resolution spectra and synthetic photometry were calculated in thewavelength range 1,000 \r{A} - 10,000 \r{A} using Non-LTE extensivelyline-blanketed atmosphere structures.

A grid of Non-LTE line-blanketed atmosphere structures and synthetic spectra for subdwarfs