MWA high frequency resolution trial observations of Galactic Centre

This dataset contains 10KHz frequency resolution observations of Galactic Centre done with MWA, plus reduced data products of this observations. This data is collected to study the potential of MWA for spectral line observations. 10 KHz resolution is not the main mode of MWA. At this stage the data set will be assessed for the quality and will serve as a testbed and reference. If the data quality is satisfactory, more observations will be planned. Separate application will be thought in such a case. High frequency resolution observations enable studying spectral line emission from galactic and extra galactic sources. Such emission may include various molecular and radio recombination lines. These spectra lines carry important information about physical conditions of the interstellar medium, and therefore allows us to understand better the evolution of stars and barionic matter in Universe.