pipeline.infrastructure.displays.plotmosaic¶
Functions
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Converts a taper in dB to the constant X in the formula FWHM=X*lambda/D for the parabolic illumination pattern. |
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Computes the scale factor of an Airy pattern as a function of the central obscuration, using Table 10.1 of Schroeder’s “Astronomical Optics”. |
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Presents a value of equatorial arc in user-friendly units. |
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Returns True if the field was only used to observe Tsys fields. |
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Labels plot axes for plots specified in units of arcseconds |
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Produce a plot of the pointings with the primary beam FWHM and field names. |
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Implements the Baars formula: b*lambda / D. |