Table B.1: Restauration errors of the reconstructions obtained with the RL, OSEM, and BB methods from the computer-simulated LBT raw images of the galaxy (see Table 1) without Fourier-masking (see Sect. 3.2).
J magnitude RL OSEM BB
16.0 $5.51\pm0.12$% $8.26\pm0.11$% $4.80\pm0.12$%
17.0 $6.36\pm0.09$% $7.55\pm0.10$% $6.16\pm0.10$%
18.0 $8.16\pm0.24$% $8.55\pm0.15$% $8.27\pm0.26$%

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 The building block method
3 Reconstruction of aperture-synthesis images from computer-simulated LBT data
4 Image reconstruction from LINC-NIRVANA data obtained with a laboratory LBT simulator
5 Space-variant Building Block method: image reconstruction from LBT raw data in the case of space-variant PSFs
6 Conclusions
References
Online Material
Appendix A: The Lagrange multiplier $\mu $ in the regularized Building Block method
Appendix B: The advantage of Fourier-masked LBT raw images
Appendix C: Space-variant BB method
List of tables
List of figures