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The influence of host galaxy morphology on the properties of Type Ia supernovae from the JLA compilation
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We study the influence of host galaxy morphology on LC parameters of the JLA data.

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The α parameter decreases from elliptical/lenticular to late-type spiral galaxies.

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In an old stellar population SNe Ia are fainter after stretch and colour corrections.

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The host galaxy morphology affects the residual dispersion on the Hubble diagram.

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SNe Ia in late-type spiral galaxies are more homogeneous in comparison with others.

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