The diffuse galactic emission maps at decimeter wavelengths (408 MHz, Haslam et al., 1982A&AS...47....1H), (1420 MHz, Reich, 1982A&AS...48..219R, Reich & Reich 1986A&AS...63..205R), (2326 MHz, Jonas et al., 1998MNRAS.297..977J) have been destriped using the method proposed by Schlegel et al., 1998ApJ...500..525S. Statistical and systematic errors have been evaluated for each map. Each map is presented in two different pixelizations: ECP (Cartesian Projection) and HEALPix. In the case of HEALPix pixelization (in which the pixel area is constant), we omitted the (constant) error maps; the statistical and systematic errors for each map are summarized in the "Table 2" section below. Synchrotron spectral index and normalization factor have been evaluated using the three destriped surveys. Some of the results in this work have been derived using the HEALPix (Gorski et al., 1999, Proceedings of the MPA/ESO Conference on Evolution of Large-Scale Structure: from Recombination to Garching, ed. A.J. Banday, R.K. Sheth, & L. Da Costa, 37).
