| DOI | Resolve DOI: https://doi.org/10.1109/ISCAS.2006.1692843 |
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| Author | Search for: Belostotski, L.; Search for: Haslett, J. W.; Search for: Veidt, Bruce1 |
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| Affiliation | - National Research Council of Canada. NRC Herzberg Institute of Astrophysics
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| Format | Text, Article |
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| Conference | 2006 IEEE International Symposium on Circuits and Systems, ISCAS 2006, 21-24 May 2006, Island of Kos, Greece |
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| Abstract | A CMOS low noise amplifier (LNA) is proposed for a proof-of-concept design of the square kilometer array (SKA) radio telescope. A novel variation on a well-known source-degenerated LNA topology is introduced that allows tuning of the power match centre frequency independently from the frequency at which the LNAs noise figure approaches its minimum noise. The 0.7-1.4 GHz LNA designed in 0.18mum CMOS achieves better than 11 dB return loss with a noise temperature of 40 K, provides a power gain of 17 dB and IP1dB of -10dBm while consuming 50 mW of power from a 1.8 V supply. The design procedure of the LNA is presented and performance of the LNA is compared with previously published results |
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| Publication date | 2006 |
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| Publisher | IEEE |
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| In | |
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| Note | yes |
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| NPARC number | 13053038 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 56cdcc1c-b8e0-4634-9940-d3060fa844be |
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| Record created | 2009-11-25 |
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| Record modified | 2020-04-22 |
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