The Telescope1D class in telescope_1d.py creates a 1 dimensional
telescope array with the specified properties. If redundant is True,
the distance between consecutive dishes is the diameter of the dishes, DDish
(i.e. a perfectly redundant array). If False, the distances are chosen
randomly from DDish, DDish*1.25, DDish*1.5, so that the array is less
redundant.
Examples of how to use this class are in telescope_1d_play.ipynb and
telescope_1d_test_foreground_filtering.
The general procedure is to initialize the telescope, create a sky
(either manually or by using the get_gaussian_sky, get_point_source_sky,
get_poisson_sky, or get_uniform_sky in the Telscope1D class).
Then, use observe_image to convolve and convert the image to uvplane (Fourier
space).
From here, you can get real space maps with error/foreground filtering
using get_obs_rmap, then get and plot the power spectra using get_rmap_ps
and plot_rmap_ps_slice.
Or, you can stay in Fourier space and get the new uvplane after adding
error/foreground filtering using get_obs_uvplane, then get and plot the power
spectra using get_uvplane_ps and plot_uvplane_ps_slice.
You can also plot the "wedge" using plot_wedge.