We explore the effect of contamination of intermediate redshift Type Ia
supernova samples by Type Ibc supernovae. Simulating observed samples of Ia and
mixed Ibc/Ia populations at a range of redshifts for an underlying cosmological
concordance model (\Omega_{m}=0.27, \Omega_{\Lambda}=0.73), we find that even
small contamination levels, 2-5% may bias the derived \Omega_{\Lambda} and
\Omega_{m} towards larger values. We thus emphasize the need for clean samples
of Type Ia SNe for accurate measurements of the cosmological parameters. We
also simulate a SN sample similar to the fiducial SNAP detected distribution
(Kim et al. 2004), but include Ibc contamination. For this distribution we
illustrate the effect of Ibc contamination on the distance modulus vs. redshift
diagram for low and high precision measurements.Comment: ApJ accepte