Abstract
In this work, spectral energy distribution has been calculated for a sample of 597 Fermi blazars. Based on the calculation, we proposed a classification for subclasses of blazars as lower synchrotron peak sources (LSPs) if [Formula: see text], intermediate synchrotron peak sources (ISPs) if [Formula: see text], higher synchrotron peak sources (HSPs) if [Formula: see text], ultra higher synchrotron peak sources (UHSPs) if [Formula: see text]. [Formula: see text]-ray luminosity is found correlated with lower energetic wavebands (radio, optical and X-rays). When redshift effect is removed, correlations are still strong for FSRQs; As for BL lacertaes, correlation between [Formula: see text]-ray and radio or between [Formula: see text]-ray and optical band is strong, but that between [Formula: see text]-ray and X-ray is only marginal.
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