Читать книгу The Doppler Method for the Detection of Exoplanets - Professor Artie Hatzes - Страница 39

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¹The focal ratio is defined as the focal length of the telescope, f, divided by its diameter, D.

²The interference pattern is merely the Fourier transform of the aperture, and as we will see in Chapter 7, there is an inverse relationship between the spatial domain and the Fourier frequency domain.

³In the 1980s, my fellow graduate student G. Donald Penrod once made the poetic remark, “There is a glorious match between CCD detectors and echelle spectrographs.” So true!