dc.contributor.author |
Saha, S. K |
|
dc.date.accessioned |
2021-02-07T04:26:13Z |
|
dc.date.available |
2021-02-07T04:26:13Z |
|
dc.date.issued |
2015 |
|
dc.identifier.citation |
xxxiii, 565p. |
en_US |
dc.identifier.isbn |
978-981-4613-27-9 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/7573 |
|
dc.description |
© Pan Stanford publishing the original publication is available at Taylor and Francis https://doi.org/10.1201/b18037 |
en_US |
dc.description.abstract |
Interferometric 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 rather |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Pan Stanford publishing |
en_US |
dc.subject |
High resolution imaging |
en_US |
dc.subject |
Technology and engineering-Mechanical |
en_US |
dc.subject |
Physical Sciences |
en_US |
dc.title |
High resolution imaging: detectors and applications |
en_US |
dc.type |
Book |
en_US |