  In this paper we determine the dipole in the distance redshift relation from
the Pantheon+ data. We find that, while its amplitude roughly agrees with the
dipole found in the cosmic microwave background which is attributed to the
motion of the solar system with respect to the cosmic rest frame, the direction
is different with a significance of slightly more than $3\si$. While the
amplitude depends on the lower redshift cutoff, the direction is quite stable.
For redshift cuts of order $z_{\rm cut} \simeq 0.05$ and higher, the dipole is
no longer detected with high statistical significance. An important r\^ole
seems to be played by the redshift corrections for peculiar velocities.
