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- W2051242998 abstract "We study the relation of Type Ia Supernovae (SNe Ia) with host galaxies from a large low redshift sample. 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 2.1{sigma}confidence level. We find that SNe Ia in high luminosity hosts are brighter after light-curve correction at>3{sigma}confidence level. We also find that SNe Ia in large size galaxies are brighter after light-curve correction at?2{sigma} confidence level. We demonstrate that the residual linearly depends on host luminosity at a confidence of 4{sigma}or host size at a confidence of 3.3{sigma}." @default.
- W2051242998 created "2016-06-24" @default.
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- W2051242998 date "2013-08-30" @default.
- W2051242998 modified "2023-09-26" @default.
- W2051242998 title "Dependence of low redshift Type Ia Supernovae luminosities on host galaxies" @default.
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- W2051242998 doi "https://doi.org/10.1088/1674-4527/13/9/007" @default.
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