The COSMOSOMAS experiment has been running for several years at the Observatorio del Teide. Since 2003 work on COSMOSOMAS has been upgraded from the usual maintenance functions to a programme of improvements as a result of renewed scientific interest in these observations. The improvements largely consist of tuning to achieve reliable data quality and improving security at the installations.
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The general goal of this project is to determine and characterize the spatial and spectral variations in the temperature and polarisation of the Cosmic Microwave Background in angular scales from several arcminutes to several degrees. The primordial matter density fluctuations which originated the structure in the matter distribution of the present