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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7573
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dc.contributor.authorSaha, S. K-
dc.date.accessioned2021-02-07T04:26:13Z-
dc.date.available2021-02-07T04:26:13Z-
dc.date.issued2015-
dc.identifier.citationxxxiii, 565p.en_US
dc.identifier.isbn978-981-4613-27-9-
dc.identifier.urihttp://hdl.handle.net/2248/7573-
dc.description© Pan Stanford publishing the original publication is available at Taylor and Francis https://doi.org/10.1201/b18037en_US
dc.description.abstractInterferometric observations need snapshots of very high time resolution of the order of (i) frame integration of about 100 Hz or (ii) photon-recording rates of several megahertz (MHz). Detectors play a key role in astronomical observations, and since the explanation of the photoelectric effect by Albert Einstein, the technology has evolved ratheren_US
dc.language.isoenen_US
dc.publisherPan Stanford publishingen_US
dc.subjectHigh resolution imagingen_US
dc.subjectTechnology and engineering-Mechanicalen_US
dc.subjectPhysical Sciencesen_US
dc.titleHigh resolution imaging: detectors and applicationsen_US
dc.typeBooken_US
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