A broadband FFT spectrometer for radio and millimeter astronomy

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Abstract

The core architecture, tests in the lab and first results of a Fast Fourier Transform (FFT) spectrometer are described. It is based on a commercially available fast digital sampler (AC240) with an on-board Field Programmable Gate Array (FPGA). The spectrometer works continuously and has a remarkable total bandwidth of 1 GHz, resolved into 16 384 channels. The data is sampled with 8 bits, yielding a dynamic range of 48 dB. An Allan time of more than 2000 s and an SFDR of 37 dB were measured. First light observations with the KOSMA telescope show a perfect spectrum without internal or external spurious signals. © ESO 2005.

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APA

Benz, A. O., Grigis, P. C., Hungerbühler, V., Meyer, H., Monstein, C., Stuber, B., & Zardet, D. (2005). A broadband FFT spectrometer for radio and millimeter astronomy. Astronomy and Astrophysics, 442(2), 767–773. https://doi.org/10.1051/0004-6361:20053568

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