Issue |
A&A
Volume 442, Number 2, November I 2005
|
|
---|---|---|
Page(s) | 767 - 773 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361:20053568 | |
Published online | 07 October 2005 |
A broadband FFT spectrometer for radio and millimeter astronomy
1
Institute of Astronomy, ETH, 8092 Zurich, Switzerland e-mail: benz@astro.phys.ethz.ch
2
Acqiris SA, 1228 Plan-les-Ouates, Switzerland
3
University of Applied Sciences Solothurn, Nordwestschweiz, Switzerland
4
ZMA, Center for Microelectronics, University of Applied Sciences Aargau, Nordwestschweiz, Switzerland
Received:
3
June
2005
Accepted:
4
July
2005
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.
Key words: instrumentation: spectrographs / methods: observational / techniques: spectroscopic / submillimeter / radio lines: stars / radio lines: general
© ESO, 2005
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