Isaac López-Fernández;Juan Daniel Gallego-Puyol;Carmen Diez;Inmaculada Malo-Gomez;Ricardo Ignacio Amils;Ralf Flückiger;Diego Marti;Ronald Hesper
{"title":"A 16-GHz Bandwidth Cryogenic IF Amplifier With 4-K Noise Temperature for Sub-mm Radio-Astronomy Receivers","authors":"Isaac López-Fernández;Juan Daniel Gallego-Puyol;Carmen Diez;Inmaculada Malo-Gomez;Ricardo Ignacio Amils;Ralf Flückiger;Diego Marti;Ronald Hesper","doi":"10.1109/TTHZ.2024.3370893","DOIUrl":null,"url":null,"abstract":"The major mm and sub-mm radio-astronomy observatories are prioritizing instantaneous bandwidth widening for their current or planned upgrades this decade. We present an ultra-wideband and ultra-low-noise cryogenic hybrid amplifier with 4 K (\n<italic>NF</i>\n = 0.06 dB) average noise temperature in the 2–18 GHz band when cooled to 6 K. It is based on a 100 nm gate pseudomorphic indium–phosphide HEMT with outstanding characteristics. This demonstration amplifier meets the noise and IF bandwidth demands of atacama large millimiter/submillimeter array (ALMA) next-generation receivers, doubling the present maximum IF instantaneous bandwidth with state-of-the-art noise performance, with a gain flatness of ±0.8 dB, and output return loss better than 15 dB over 85% of the band. It can be used in the 1–19 GHz range with negligible degradation, and a tentative test has been performed with a 602–720 GHz ALMA band-9 double sideband SIS mixer, showing a flat-average and low-ripple IF noise level in an 18-GHz wideband down to near dc. A balanced configuration is feasible to improve the input matching.","PeriodicalId":13258,"journal":{"name":"IEEE Transactions on Terahertz Science and Technology","volume":"14 3","pages":"336-345"},"PeriodicalIF":3.9000,"publicationDate":"2024-02-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=10449381","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"IEEE Transactions on Terahertz Science and Technology","FirstCategoryId":"5","ListUrlMain":"https://ieeexplore.ieee.org/document/10449381/","RegionNum":2,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ENGINEERING, ELECTRICAL & ELECTRONIC","Score":null,"Total":0}
引用次数: 0
Abstract
The major mm and sub-mm radio-astronomy observatories are prioritizing instantaneous bandwidth widening for their current or planned upgrades this decade. We present an ultra-wideband and ultra-low-noise cryogenic hybrid amplifier with 4 K (
NF
= 0.06 dB) average noise temperature in the 2–18 GHz band when cooled to 6 K. It is based on a 100 nm gate pseudomorphic indium–phosphide HEMT with outstanding characteristics. This demonstration amplifier meets the noise and IF bandwidth demands of atacama large millimiter/submillimeter array (ALMA) next-generation receivers, doubling the present maximum IF instantaneous bandwidth with state-of-the-art noise performance, with a gain flatness of ±0.8 dB, and output return loss better than 15 dB over 85% of the band. It can be used in the 1–19 GHz range with negligible degradation, and a tentative test has been performed with a 602–720 GHz ALMA band-9 double sideband SIS mixer, showing a flat-average and low-ripple IF noise level in an 18-GHz wideband down to near dc. A balanced configuration is feasible to improve the input matching.
期刊介绍:
IEEE Transactions on Terahertz Science and Technology focuses on original research on Terahertz theory, techniques, and applications as they relate to components, devices, circuits, and systems involving the generation, transmission, and detection of Terahertz waves.