5 Conclusion

We presented a new, sophisticated instrument for multi-dimensional spectroscopy, consisting of the scanning device MISC, a Stokes-V polarimeter and a fast CCD camera. Since its first preliminary installation at the GCT in July 1995, it has been in regular use and provides a wealth of data. The handling of the data and the first results will be discussed in a forthcoming publication.

Acknowledgements

We thank the mechanical and electronic workshops of the Universitäts-Sternwarte Göttingen where most of the hardware was designed and constructed. Advice from "La Vision 2D-Meßtechnik'' is gratefully acknowledged.

The Gregory Coudé Telescope is operated by the Universitäts-Sternwarte Göttingen at the Spanish Observatorio del Teide of the Instituto de Astrofísica de Canarias. This work was supported by the Deutsche Forschungsgemeinschaft, through grant Kn 152/16-1,-2.