- Figure 1: The black disk is the ber and the light ring is the light from the star outside the ber. Very precise centering is possible as can be seen, and the NOT guide system was shown
- FIES: A high resolution FIber fed Echelle Spectro-graph for NOT
- 5HSRUW IRU WKH 127 67& RQ WKH ),(6 6SHFWURJUDSK #6XSSOHPHQW WR WKH UHSRUW GDWHG ###########
- Institute of Astronomy, University of Vienna Delta Scuti Star Newsletter, Vol. 16?, 2001
- A new High Resolution Spectrograph at the NOT Sren Frandsen
- Fig. 1.---The layout of the fiber optics, which permit to set the object on the fiber and guide very accurately. The fiber is to the right, the standby CCD camera to the left. The previous mirror, situated on the connection
- Measuring Oscillations in Nearby Stars (MONS): status spring 2001 Sren Frandsen
- Institute of Astronomy, University of Vienna Delta Scuti Star Newsletter, Vol. 16?, 2001
- Astronomy & Astrophysics manuscript no. (will be inserted by hand later)
- Radial and Nonradial Pulsations as Probes of Stellar Physics ASP Conference Series, Vol. 259, 2002
- Basic ESP Activation 1. Log on as root
- MONS: Technical development and groundbased support observations Sren Frandsen
