The Multi-Unit Spectroscopic Explorer (MUSE) samples almost the
full optical domain with a mean resolution of 3000. The instrument has
a modular structure composed of 24 identical IFU. It covers nearly 1
squared arcmin field of view in the Wide Field Mode (WFM) and 7.5
squared arcsec field of view in the Narrow Field Mode (NFM). MUSE was
commissioned in the first half of 2014 and became operational in
October 2014 (P94). These pages contain information about MUSE Quality
Control, pipeline processing, and data flow operations.
quyality-controlled and homogeneous processing of entire data history into spectral data products (not flux-calibrated); new data are added about monthly