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Redshifts of supernova (SN) and gamma‐ray burst (GRB) samples are compared with the pixel temperatures of the  Wilkinson Microwave Anisotropy Probe  ( WMAP ) seven‐year data, the pixel locations corresponding to the SN and GRB sky coordinates. We have found a statistically significant correlation of the SN redshifts with the  WMAP  data, the average temperature deviation being  for redshifts  z  ranging from 0.5 to 1.0 and  for  z ∈ (0.0, 0.4). The latter value accords with the theoretical estimates for the distortion of the cosmic microwave background due to the integrated Sachs–Wolfe effect, whereas the larger anomaly for higher redshifts should be studied in more detail in the future.

Correlation of supernova redshifts with temperature fluctuations of the cosmic microwave background