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- W2078550936 abstract "To image astronomical objects, the Hanbury Brown Twiss (HBT) technique involves measuring intensity correlation foran array of telescopes. The correlation of the intensity fluctuations is a measure of the magnitude of the coherence andcan be used to retrieve the intensity distribution of the source using the Van Cittert-Zernike theorem. For low spectralirradiance sources, coincidence counting using modern techniques can drastically reduce data storage/processingrequirements as well as allowing for optimization of the effective SNR bandwidth. In counting Intensity Interferometry(II), count fluctuations are measured instead of intensity fluctuations as with an analog II. Those are the two IItechniques currently reported in the literature. Since the successful width measurements of bright stars by HBT in the70's, advances in detectors promise opportunities to apply II to dimmer non-point source objects. To improve SNRs, wepropose a new data processing technique for measuring correlation in the low light regime that ensures maximumbandwidth allowed by the reproducibility of photon pulses." @default.
- W2078550936 created "2016-06-24" @default.
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- W2078550936 date "2011-05-13" @default.
- W2078550936 modified "2023-09-23" @default.
- W2078550936 title "Improved correlation determination for intensity interferometers" @default.
- W2078550936 doi "https://doi.org/10.1117/12.883405" @default.
- W2078550936 hasPublicationYear "2011" @default.
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