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PURIFY
Next-generation radio interferometric imaging
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Go to the source code of this file.
Namespaces | |
purify | |
purify::widefield | |
Functions | |
t_int | purify::widefield::w_support (const t_real w, const t_real du, const t_int min, const t_int max) |
estimate support size of w given u resolution du More... | |
t_real | purify::widefield::pixel_to_lambda (const t_real cell, const t_uint imsize, const t_real oversample_ratio) |
return factors to convert between arcsecond pixel size image space and lambda for uv space More... | |
t_real | purify::widefield::estimate_cell_size (const t_real max_u, const t_uint imsize, const t_real oversample_ratio) |
return cell size from the bandwidth More... | |
t_real | purify::widefield::fov_cosine (t_real const cell, t_uint const imsize) |
Work out max L and M directional cosines from image parameters. More... | |
t_real | purify::widefield::equivalent_miriad_cell_size (const t_real cell, const t_uint imsize, const t_real oversample_ratio) |
for a given purify cell size in arcsec provide the equivalent miriad cell size in arcsec More... | |
Matrix< t_complex > | purify::widefield::generate_chirp (const t_real w_rate, const t_real cell_x, const t_real cell_y, const t_uint x_size, const t_uint y_size) |
Generates image of chirp. More... | |
Matrix< t_complex > | purify::widefield::estimate_sample_density (const Vector< t_real > &u, const Vector< t_real > &v, const t_real cellx, const t_real celly, const t_uint imsizex, const t_uint imsizey, const t_real oversample_ratio, const t_real scale) |
estimate sample desity grid for a given field of view More... | |
Vector< t_complex > | purify::widefield::sample_density_weights (const Vector< t_real > &u, const Vector< t_real > &v, const t_real cellx, const t_real celly, const t_uint imsizex, const t_uint imsizey, const t_real oversample_ratio, const t_real scale) |
create sample density weights for a given field of view, uniform weighting More... | |