  We report a serendipitous hard X-ray (3-24 keV) detection of the blazar LBQS
1319+0039. The X-ray spectrum is consistent with powerlaw emission with a
photon index of $\Gamma = 1.78$. The observed emission and published redshift
imply an observed 2-10 keV luminosity of $3.4\times10^{45}$ erg s$^{-1}$. This
is consistent with extrapolations from a previous soft X-ray detection, thus
there is no evidence for strong variability.
