Abstract
We explore the effect of contamination of intermediate-redshift Type Ia supernova samples by Type Ibc supernovae (SNe). Simulating observed samples of Type Ia and mixed Type Ibc/Ia populations at a range of redshifts for an underlying cosmological concordance model (ΩM = 0.27, Ωλ = 0.73), we find that even small contamination levels, 2%-5%, may bias the derived Ωλ and ΩM toward 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 of Kim and coworkers, but include Type Ibc contamination. For this distribution we illustrate the effect of Type Ibc contamination on the distance modulus versus redshift diagram for low- and high-precision measurements.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
