The zoomed frame (lower right) shows the image of a single Argon
spectral line through the object and sky fiber.
The respective two half images due to the
image slicer are clearly seen. The FWHM in dispersion (= y-)direction
is measured to 33 micron, i.e., 2.2 pixels on the final 15 mu pixel
Therefore, the full spectral resolving power of R = 48000 was obtained with the first test images !
If you have any comments on the FEROS project, please send me a mail .
FEROS homepage / A.Kaufer@lsw.uni-heidelberg.de Last modified: Fri Jan 26 10:37:19 MET 2001