High-resolution radio observations of Seyfert galaxies in the extended 12-micron sample - I. The Observations

Abstract

We present 8.4 GHz VLA A–configuration observations of 87 sources from the mid–infrared–selected AGN sample of Rush et al. (1993). These 0.25 arcsec resolution observations allow elongated radio structures tens of parsecs in size to be resolved and enable radio components smaller than 3.5 arcsec to be isolated from diffuse galactic disc emission. When combined with previous data, matched radio observations covering ninety percent of the sample have been collected and these represent the largest sub–arcsecond–resolution radio imaging survey of a homogeneously–selected sample of Seyfert galaxies to date. We use our observations to identify 5 radio–loud AGN in the sample. The nature of the radio emission from Seyfert nuclei will be discussed in subsequent papers.