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We present a proposal for the construction and development of a newinstrument for radio astronomical observations based on interferometrictechniques, that will provide high angular resolution in the 21 cm band, withthe intention of improving and extending the current performance of theinstruments used at the Argentine Institute of Radio Astronomy. This will allowinternationally competitive scientific research and the acquisition ofcutting-edge scientific and technological know-how in the aforementionedtechniques, enabling interferometric measurements and the development of verylong baseline or VLBI techniques. This project is called MIA, an acronym for"Multipurpose Interferometric Array".

The Multipurpose Interferometric Array and the development of its technological demonstrator