“…The few small ( 10 element) heterodyne arrays that have been realized in the submil-limeter rely on close packing individual single pixel waveguide receivers with non optimal fill-factors [5,6,7,8]. Several clever millimeter wave array systems have been constructed in W-band (generally centered around the 94 GHz atmospheric window) but all are fairly bulky and expensive [9,10,11,12,13]. Focal plane direct detection arrays are much easier to realize in this frequency range for the reasons stated, (no LO and simple DC output) and there are many viable designs from the late 1980's to the mid 1990's for submillimeter-wave array concepts developed largely for the radio astronomy community [14,15,16,17,18,19,].…”