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- W3146976800 abstract "We study the relation between Type Ia Supernovae(SNe Ia) and properties of their host galaxies using a large sample with low redshift. By examining the Hubble residuals of the entire sample from the best-fit cosmology, we show that SNe Ia in passive hosts are brighter than those in star-forming hosts after light curve correction at the 2.1σ confidence level. We find that SNe Ia in high luminosity hosts are brighter after light-curve correction at the > 3σ confidence level. We also find that SNe Ia in large galaxies are brighter after light-curve correction at the≥2σ confidence level. We demonstrate that the residuals depend linearly on host luminosity at a confidence of 4σ or host size at a confidence of 3.3σ." @default.
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- W3146976800 date "2013-01-01" @default.
- W3146976800 modified "2023-09-23" @default.
- W3146976800 title "Dependence of low redshift Type Ia Supernovae luminosities on host galaxies" @default.
- W3146976800 hasPublicationYear "2013" @default.
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