The following document lists the file abstract/MGERIN_DUST_Z.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
===================================================================== == In this proposal, more time is being requested for MGERIN.DUST_HIZ == The sample has been enlarged and the instrumental configuration changed. ===================================================================== We propose in this proposal to investigate the dust properties of distant IRAS galaxies (z =0.3, 0.6, 0.93 and 2.6) by looking for the presence of the UIBs in their spectrum. The presence of these features and the detailed spectrum will give a good assessment on the nature of dust grains in these distant galaxies. We shall also measure the overall shape of the spectrum in the infrared, a very important ingredient in the interpretation of faint galaxy counts and in the prediction of the extragalactic background in the infrared.