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We present a model independent analysis of the Pantheon+ supernova sample and study the dependence of the recovered values of $H_0$, $q_0$ and $j_0$ on the redshift cut and on the modeling of peculiar velocities.
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A. Carr, T. M. Davis, D. Scolnic, K. Said, D. Brout, E. R. Peterson, and R. Kessler, The pantheon+ analysis: Improving the redshifts and peculiar velocities of type ia supernovae used in cosmological analyses
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L. Perivolaropoulos and F. Skara, On the homogeneity of SnIa absolute magnitude in the Pantheon+ sample
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F. Sorrenti, R. Durrer, and M. Kunz, The low multipoles in the Pantheon+SH0ES data
Cited in the paper.
E. O. Lebigot, “Uncertainties: a python package for calculations with uncertainties.” http://pythonhosted.org/uncertainties/
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