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Identifying variable gamma-ray sources through radio observations

J. M. Paredes, J. Marti, D. F. Torres, G. E. Romero, J. A. Combi, V. Bosch-Ramon, J. Garcia-Sanchez

astro-pharXiv:astro-ph/0407454

Abstract

We present preliminary results of a campaign undertaken with different radio interferometers to observe a sample of the most variable unidentified EGRET sources. We expect to detect which of the possible counterparts of the gamma-ray sources (any of the radio emitters in the field) varies in time with similar timescales as the gamma-ray variation. If the gamma-rays are produced in a jet-like source, as we have modelled theoretically, synchrotron emission is also expected at radio wavelengths. Such radio emission should appear variable in time and correlated with the gamma-ray variability.

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