We present two-dimensional hydrodynamics simulations of near-Chandrasekhar mass white dwarf ( WD ) models for Type Ia supernovae ( SNe Ia ) using the turbulent deflagration model with deflagration-detonation transition ( DDT ) . We perform a parameter survey for 41 models to study the effects of the initial central density ( i.e. , WD mass ) , metallicity , flame shape , DDT criteria , and turbulent flame formula for a much wider parameter space than earlier studies . The final isotopic abundances of ^ { 11 } C to ^ { 91 } Tc in these simulations are obtained by post-process nucleosynthesis calculations . The survey includes SNe Ia models with the central density from 5 \times 10 ^ { 8 } g cm ^ { -3 } to 5 \times 10 ^ { 9 } g cm ^ { -3 } ( WD masses of 1.30 - 1.38 M _ { \odot } ) , metallicity from 0 to 5 Z _ { \odot } , C/O mass ratio from 0.3 - 1.0 and ignition kernels including centered and off-centered ignition kernels . We present the yield tables of stable isotopes from ^ { 12 } C to ^ { 70 } Zn as well as the major radioactive isotopes for 33 models . Observational abundances of ^ { 55 } Mn , ^ { 56 } Fe , ^ { 57 } Fe and ^ { 58 } Ni obtained from the solar composition , well-observed SNe Ia and SN Ia remnants are used to constrain the explosion models and the supernova progenitor . The connection between the pure turbulent deflagration model and the subluminous SNe Iax is discussed . We find that dependencies of the nucleosynthesis yields on the metallicity and the central density ( WD mass ) are large . To fit these observational abundances and also for the application of galactic chemical evolution modeling , these dependencies on the metallicity and WD mass should be taken into account .