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NGC 7582 was identified as a Starburst galaxy in the optical \cite[(Veron etal. 1981)]{Veron et al.(1981)} but its X-Ray emission is typical of a Seyfert 1galaxy \cite[(Ward et al. 1978)]{Ward et al.(1978)}. We analyzed a datacube ofthis object obtained with the GMOS-IFU on the Gemini-South telescope. After asubtraction of the stellar component using the {\sc starlight} code \cite[(CidFernandes et al. 2005)]{Cid Fernandes et al. (2005)}, we looked for opticalsignatures of the AGN. We detected a broad $H\alpha$ component (figure\ref{fig1}) in the source where \cite[Bianchi et al.(2007)]{Bianchi etal.(2007)} identified the AGN in an HST optical image. We also found a broad$H\beta$ feature (figure \ref{fig2}), but its emission reveals a extendedsource. We suggest that it is the light of the AGN scattered in the ionizationcone. We propose that NGC 7582 is a Seyfert 1 galaxy. A number of other"hot-spots" and Wolf-Rayet features were also identified.

The AGN properties of the starburst galaxy NGC 7582