arXiv · astro-ph/0610580
The optical performance of frequency selective bolometers
Abstract
Frequency Selective Bolometers (FSBs) are a new type of detector for millimeter and sub-millimeter wavelengths that are transparent to all but a narrow range of frequencies as set by characteristics of the absorber itself. Therefore, stacks of FSBs tuned to different frequencies provide a low-loss compact method for utilizing a large fraction of the light collected by a telescope. Tests of prototype FSBs, described here, indicate that the absorption spectra are well predicted by models, that peak absolute absorption efficiencies of order 50% are attainable, and that their out-of-band transmission is high.
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T. A. Perera, T. C. Chen, E. S. Cheng, D. A. Cottingham, T. M. Crawford, T. P. Downes, F. M. Finkbeiner, D. J. Fixsen, D. W. Logan, S. S. Meyer, E. H. Sharp, R. F. Silverberg, G. W. Wilson. 2006-10-19. The optical performance of frequency selective bolometers. https://doi.org/10.1364/ao.45.007643
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