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Low-noise 6-8 GHz receiver

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dc.contributor.authorPandian, J D
dc.contributor.authorBaker, L
dc.contributor.authorCortes, G
dc.contributor.authorGoldsmith, P F
dc.contributor.authorDeshpande, A A
dc.contributor.authorGanesan, R
dc.contributor.authorHagen, J
dc.contributor.authorLocke, L
dc.contributor.authorWadefalk, N
dc.contributor.authorWeinreb, S
dc.date.accessioned2007-03-16T10:07:34Z
dc.date.available2007-03-16T10:07:34Z
dc.date.issued2006-12
dc.descriptionOpen Access.en
dc.description.abstractThe combination of the traveling wave OMT device and the ultra-low-noise MMIC amplifiers has allowed us to develop a broadband 6-8 GHz receiver with a noise temperature of around 10 K. The combination of receiver noise and the additional noise contributions by the telescope optics gives an overall receiver temperature of around 28 K and 34 K in the two polarizations. The large collecting area of the telescope gives rise to a system equivalent flux density of around 4.5 Jy at 7 GHzen
dc.format.extent3601165 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationIEEE Microwave Magazine, 2006, Vol.7, p74-84en
dc.identifier.issn1527-3342
dc.identifier.urihttp://hdl.handle.net/2289/2212
dc.language.isoenen
dc.publisherIEEEen
dc.relation.urihttp://dx.doi.org/10.1109/MW-M.2006.250316en
dc.rights© 2006 IEEE. This material is posted here with permission of the IEEE. Such permission of the IEEE does not in any way imply IEEE endorsement of any of Raman Research Institute's's products or services. Internal or personal use of this material is permitted. However, permission to reprint/republish this material for advertising or promotional purposes or for creating new collective works for resale or redistribution must be obtained from the IEEE by writing to pubs-permissions@ieee.org. By choosing to view this document, you agree to all provisions of the copyright laws protecting it.en
dc.titleLow-noise 6-8 GHz receiveren
dc.typeArticleen

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