Abstract
In this paper we present a new spectrophotometer ESOP (Experience Spectroscopique d'Observation des Plasmas). We describe its general features and characteristics. We report the first spectrophotometric results on the Puppis A supernova remnant on the coronal iron line emission. These [FeXIV] observations were in the vicinity of the “Eastern X-ray knot.” We have observed at 30″ scale. In appendices we describe in more details some specific technical points.
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