Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/8074
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dc.contributor.authorGirish, B.S.-
dc.contributor.authorReddy, S. Harshavardhan-
dc.contributor.authorSethi, Shiv-
dc.contributor.authorSrivani, K.S.-
dc.contributor.authorAbhishek, R.-
dc.contributor.authorAjithkumar, B.-
dc.contributor.authorBhattramakki, Sahana-
dc.contributor.authorBuch, Kaushal-
dc.contributor.authorChaudhuri, Sandeep-
dc.contributor.authorGupta, Yashwant-
dc.contributor.authorKamini, P.A.-
dc.contributor.authorKudale, Sanjay-
dc.contributor.authorMadhavi, S.-
dc.contributor.authorMuley, Mekhala-
dc.contributor.authorPrabu, T.-
dc.contributor.authorRaghunathan, A.-
dc.contributor.authorShelton, G.J.-
dc.date.accessioned2023-04-03T09:19:57Z-
dc.date.available2023-04-03T09:19:57Z-
dc.date.issued2023-03-31-
dc.identifier.citationJournal of Astrophysics and Astronomy, 2023, Vol. 44, Article No. 28en_US
dc.identifier.issn0250-6335-
dc.identifier.issn0973-7758 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/8074-
dc.descriptionOpen Access from Indian Academy of Sciencesen_US
dc.description.abstractBacked by advances in digital electronics, signal processing, computation and storage technologies, aperture arrays, which had strongly influenced the design of telescopes in the early years of radio astronomy, have made a comeback. Amid all these developments, an international effort to design and build the world’s largest radio telescope, the Square Kilometre Array (SKA), is ongoing. With its vast collecting area of 1 km2 , the SKA is envisaged to provide unsurpassed sensitivity and leverage technological advances to implement a complex receiver to provide a large field of view through multiple beams on the sky. Many pathfinders and precursor aperture array telescopes for the SKA, operating in the frequency range of 10–300 MHz, have been constructed and operationalized to obtain valuable feedback on scientific, instrumental and functional aspects. This review article looks explicitly into the progression of digital-receiver architecture from the Murchison Widefield Array (precursor) to the SKA1-Low. It highlights the technological advances in analog-to-digital converters (ADCs), field-programmable gate arrays (FPGAs) and central processing unit–graphics processing unit (CPU–GPU) hybrid platforms around which complex digital signal processing systems implement efficient channelizers, beamformers and correlators. The article concludes with a preview of the design of a new generation signal processing platform based on radio frequency system-on-chip (RFSoC).en_US
dc.language.isoenen_US
dc.publisherIndian Academy of Sciencesen_US
dc.relation.urihttps://doi.org/10.1007/s12036-023-09921-3en_US
dc.rights2023 Indian Academy of Sciences, Bengaluruen_US
dc.titleProgression of digital-receiver architecture: From MWA to SKA1-Low, and beyonden_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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