new_fits = fits.open(new_fitsname, mode='update')
write_every = 10000
vel_res = cube._pix_size_slice(0) * u.m / u.s
print("And here we go!")
for num, (i, j) in enumerate(ProgressBar(zip(*posns))):
# Don't bother rolling if there's nothing there
if not np.isfinite(cube.filled_data[:, i, j]).any():
continue
shift = ((model[0].data[i, j] * u.m / u.s - vsys) / vel_res).value
new_fits[0].data[:, i, j] = \
fourier_shift(cube.filled_data[:, i, j], shift)
# Now shift the source mask by the same amount
# Gibbs ringing occurs at the edges, but the amplitudes will not
# exceed 0.5. The rounding may cause a difference os +/- on pixel
# one the edge of the valid regions.
mask.data[:, i, j] = \
(fourier_shift(mask.data[:, i, j], shift) > 0.5).astype(np.int)
if num % write_every == 0:
new_fits.flush()
# Save the rotation subtracted mask
new_mask_hdu = fits.PrimaryHDU(mask.data, header=mask.header)
new_mask_hdu.writeto(fourteenB_HI_data_path(rotsub_mask_name, no_check=True),
clobber=True)
if os.path.exists(new_fitsname):
print("Removing old rotsub version.")
os.system("rm {}".format(new_fitsname))
create_huge_fits(new_fitsname, new_header)
new_fits = fits.open(new_fitsname, mode='update')
write_every = 20000
vel_res = cube._pix_size_slice(0) * u.m / u.s
vsys = gal.vsys.to(u.m / u.s)
print("And here we go!")
for num, (i, j) in enumerate(ProgressBar(zip(*posns))):
# Don't bother rolling if there's nothing there
if not np.isfinite(cube.filled_data[:, i, j]).any():
continue
shift = ((model[i, j] * u.m / u.s - vsys) / vel_res).value
new_fits[0].data[:, i, j] = \
fourier_shift(cube.filled_data[:, i, j], shift)
if num % write_every == 0:
new_fits.flush()
new_fits.flush()
new_fits.close()
