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We use a recent Pantheon+SH0ES compilation of Type Ia Supernova distance measurements at low-redshift, i.e., $0.01 \leq z \leq 0.10$, in order to investigate the directional dependency of the deceleration parameter ($q_0$) in different patches ($60^{\circ}$ size) across the sky, as a probe of the statistical isotropy of the Universe.
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F. Sorrenti, R. Durrer and M. Kunz, “The dipole of the Pantheon+SH0ES data,” JCAP 11
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