Probing the nature of compact ultra-steep spectrum radio sources with the e-EVN and e-MERLIN

Abstract

We present first results from electronic Multi-Element Remotely Linked Interferometer Network (e-MERLIN) and electronic European VLBI Network (e-EVN) observations of a small sample of ultra-steep spectrum radio sources, defined as those sources with a spectral index alpha < -1.4 between 74 MHz and 325 MHz, which are unresolved on arcsecond scales. Such sources are currently poorly understood and a number of theories as to their origin have been proposed in the literature. The new observations described here have resulted in the first detection of two of these sources at milliarcsecond scales and show that a significant fraction of ultra-steep spectrum sources may have compact structures which can only be studied at the high resolution available with very long baseline interferometry (VLBI).

Five pages, two tables, one figure. Accepted to MNRAS Letters

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• The e-MERLIN Data Reduction Pipeline
• High-Resolution Radio Observations of Five Optically Selected Type 2 Quasars