Commit b53acb4e authored by Emanuele De Rubeis's avatar Emanuele De Rubeis
Browse files

Allows to plot fits files produced as output

parent 45e27c45
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+32 −0
Original line number Diff line number Diff line
#!/usr/bin/python3
import numpy as np
import matplotlib.pyplot as plt
from astropy.io import fits
real_fits = "/home/emanuele/hpc_imaging/test_fits_real.fits"
imag_fits = "/home/emanuele/hpc_imaging/test_fits_img.fits"
nplanes = 1


with fits.open(real_fits) as hdu_real:
	img_hdu_real = np.array(hdu_real[0].data)

with fits.open(imag_fits) as hdu_imag:
	img_hdu_imag = np.array(hdu_imag[0].data)


xaxis = int(np.sqrt(img_hdu_real.size))
yaxes = xaxis
residual = np.vectorize(complex)(img_hdu_real, img_hdu_imag)

cumul2d = residual.reshape((xaxis,yaxes,nplanes), order='F')

for i in range(nplanes):
    gridded = np.squeeze(cumul2d[:,:,i])
    ax = plt.subplot()
    img = ax.imshow(np.abs(np.fft.fftshift(gridded)), aspect='auto', interpolation='none', origin='lower')
    ax.set_xlabel('cell')
    ax.set_ylabel('cell')
    cbar = plt.colorbar(img)
    cbar.set_label('norm(FFT)',size=18)
    figname='fits_image_' + str(i) + '.png'
    plt.savefig(figname)