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Proceedings ArticleDOI

Digitizing The Yuan Tseh Lee Array for Microwave Background Anisotropy by 5Gsps ADC boards

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TLDR
An 8 bits, 5 Giga samples per second Analog to Digital Printed Circuit Board has been designed by the authors for digitizing The Yuan Tseh Lee Array for Microwave Background Anisotropy and other radio telescopes.
Abstract
An 8 bits, 5 Giga samples per second Analog to Digital Printed Circuit Board has been designed by the authors for digitizing The Yuan Tseh Lee Array for Microwave Background Anisotropy(AMiBA) and other radio telescopes. Associated with the Field Programmable Gate Array platform developed by the Collaboration for Astronomy Signal Processing and Electronics Research community, AMiBA will have a digital correlator system in the future, that was fiscally difficult in 2001 when it was at design phase. The board can digitize input radio frequencies from DC up to 2.5GHz with a flatness of 5dB. The ENOB ranges from 6.1 to 6.5 bits across the 2.5GHz band, the SFDR from 41 dB to 48 dB, and the SINAD from 32 dB to 37.5 dB if the gain and offset tuning is applied.

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Proceedings ArticleDOI

Design of an interim digital spectro-correlator for the Yuan Tseh Lee array for microwave background anisotropy

TL;DR: The laboratory design and implementation of a four-antenna digital spectro-correlator for the Yuan Tseh Lee Array for Microwave Background Anisotropy (AMiBA) enables the AMiBA for new scientific missions, such as CO intensity mapping.
Proceedings ArticleDOI

The design of a10-Gsps analog-to-digital converter board for the radio astronomy community

TL;DR: A 4-bit, 10 gigasamples per second analog-to-digital converter (ADS) printed circuit board (PCB) was designed and manufactured for digitizing radio telescopes and provides data acquisition systems with a wider bandwidth and simplifies the intermediate frequency (IF) section.
References
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Journal ArticleDOI

New SETI Sky Surveys for Radio Pulses

TL;DR: Astropulse and Fly's Eye as discussed by the authors are two of the most popular SETI programs at IR, visible and radio wavelengths, which are orthogonal in search space; the Allen Telescope Array (ATA) “Fly's Eye” experiment observes a 100 square degree field by pointing each 6m ATA antenna in a di erent direction.
Journal ArticleDOI

The Yuan-Tseh Lee Array for microwave background anisotropy

TL;DR: The Yuan-Tseh Lee Array for microwave background anisotropy is the first interferometer dedicated to study the cosmic microwave background radiation at 3 mm wavelength as discussed by the authors, where the choice of 3 mm is to minimize the contributions from foreground synchrotron radiation and Galactic dust emission.
Proceedings ArticleDOI

DA and AD converters in SiGe technology: Speed and resolution for ultra high data rate applications

TL;DR: DA and AD converters are key elements for implementing new modulation formats in next generation optical transport systems and latest results and future trends are presented with a focus on SiGe devices.
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