The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards.
I. NLTE spectral analysis of the DA-type white dwarf G 191-B2B
Rauch et al. 2013, A&A 560, A104.
These two figures show a comparison of our final model with the observation in the FUSE (910 - 1188 Å) and STIS (1150 - 1780 Å) wavelength range.
An animated comparison of an HST/STIS observation of the DA-type white dwarf G191-B2B with grating E140H (resolving power R = 114 000) with the final model of Rauch et al. 2013 can be found here.
