A compact radio source in the high-redshift soft gamma-ray blazar IGR
  J12319-0749
  Context. Blazars are powerful active galactic nuclei (AGNs) radiating
prominently in the whole electromagnetic spectrum, from the radio to the X-ray
and gamma-ray bands. Their emission is dominated by synchrotron and
inverse-Compton radiation from a relativistic jet originating from an accreting
central supermassive black hole. The object IGR J12319-0749 has recently been
identified as a soft gamma-ray source with the IBIS instrument of the INTEGRAL
satellite, coincident with a quasar at high redshift (z=3.12). Aims. We studied
the radio structure of IGR J12319-0749 to strengthen its blazar identification
by detecting a compact radio jet on the milli-arcsecond (mas) angular scale,
and to measure its astrometric position accurate to mas level. Methods. We used
the technique of electronic very long baseline interferometry (e-VLBI) to image
IGR J12319-0749 with the European VLBI Network (EVN) at 5 GHz on 2012 June 19.
Results. IGR J12319-0749 (J1231-0747) is a compact radio source, practically
unresolved on interferometric baselines up to ~136 million wavelengths. The
estimated brightness temperature (at least ~2 x 10^12 K) indicates that the
radio emission of its jet is Doppler-boosted. The accurate position of the
compact radio source is consistent with the positions measured at higher
energies.
