We present the search for different Type Ia Supernovae (SNe Ia) by host-galaxy from a larger low redshift sample. We examine the residuals of the entire sample from the best-fit cosmology and find that at 2.1sigm confidence level, SNe Ia in passive hosts are brighter than those in star-forming hosts after light curve correction. We present an evidence that has a correlation (3 sigm confidence level) between the residuals of SNe Ia about the best-fit Hubble relation and their host galaxy size or luminosity, in which SNe Ia are brighter in brighter or bigger hosts.
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