We have developed a 4 x 8 array of stressed Ge:Ga detectors. This array det
ector has a high density format of entrance pupils so that we can minimize
the size of the camera optics. The cutoff wavelength of the detector is abo
ut 170 mu m, and the detector's NEP is better than 10(16) W Hz(-1/2). We ar
e going apply this array detector to balloon-borne astronomical observation
s. Furthermore, we are developing this detector into a 5 x 15 array detecto
r that will be placed onboard the IRIS satellite to be launched in 2003.