Fit All Spectra with Default Parameters
In ELFO, the process_i and process_j functions use the default parameter file
qsopar_muse.fits to fit an entire row of spectra. You can refer to the example file on the PyQSOFit website
for guidance on how to create this file. To fit all spectra, you may refer to the code below.
1for i in range(npixel):
2 process_i(i, path_out, wave, flux_cube, var_cube, 0.05668, ra, dec, path_ex)
3
4 # or
5
6for j in range(npixel):
7 process_j(j, path_out, wave, flux_cube, var_cube, 0.05668, ra, dec, path_ex)
The effect of the code is the same as using a simple for loop with PyQSOFit to fit each pixel. However, the function here uses multiprocessing to perform the fitting, which will be more efficient.