JWST related studies by Wolfram Freudling

Optimal Size of Spectrograph Pixels for Galaxy Surveys (Sep 2001)
Slit-losses as function of Magnitude for faint HDF Galaxies (Oct 2001)
Efficiency of Spectrograph with Slits formed of MEMS (Nov 2001)
Crowding of NIRSPEC spectra, (AAS poster by Freudling, Arribas, Cristiani, Fosbury, Jakobsen, Pirzkal, Jan 2002), ISR, in preparation
Sizes of HDF NICMOS galaxies at the magnitude limit of NIRSPEC (Feb 2002)
Throughput of MEMS generated SLIT as a function of Dither Positions (March 2002)
Throughput of MEMS generated SLIT as a function of Size of Spectrograph entrance pupil (March 2002)
The Cost of Dithering with NIRSPEC (July 2002)
Centering of Target on MEMS Slit (Dec 2002)