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We probe the possible anisotropy of the Universe by using the JLA compilation of type-Ia supernovae. We apply the Markov Chain Monte Carlo (MCMC) method to constrain the amplitude and direction of anisotropy in three cosmological models. For the dipole-modulated CDM model, the anisotropic amplitude is consistent with zero at C.L., and has an upper bound at C.L. Regardless of much larger uncertainty, we find the dipole direction of JLA is amazingly opposite to that of Union2. Similar results are found for the dipole-modulated CDM and CPL models. Thus, the Universe is still well consistent with the isotropy according to the JLA compilation.

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