revamp imagerie
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@@ -20,17 +20,17 @@ from astropy.wcs import WCS
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def main():
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##### User inputs
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## Input and output locations
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globals()['data_folder'] = "../data/NGC1068_x274020/"
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infiles = ['x274020at.c0f.fits','x274020bt.c0f.fits','x274020ct.c0f.fits',
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'x274020dt.c0f.fits','x274020et.c0f.fits','x274020ft.c0f.fits',
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'x274020gt.c0f.fits','x274020ht.c0f.fits','x274020it.c0f.fits']
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psf_file = 'NGC1068_f253m00.fits'
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globals()['plots_folder'] = "../plots/NGC1068_x274020/"
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# globals()['data_folder'] = "../data/NGC1068_x274020/"
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# infiles = ['x274020at.c0f.fits','x274020bt.c0f.fits','x274020ct.c0f.fits',
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# 'x274020dt.c0f.fits','x274020et.c0f.fits','x274020ft.c0f.fits',
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# 'x274020gt.c0f.fits','x274020ht.c0f.fits','x274020it.c0f.fits']
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## psf_file = 'NGC1068_f253m00.fits'
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# globals()['plots_folder'] = "../plots/NGC1068_x274020/"
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# globals()['data_folder'] = "../data/IC5063_x3nl030/"
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# infiles = ['x3nl0301r_c0f.fits','x3nl0302r_c0f.fits','x3nl0303r_c0f.fits']
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globals()['data_folder'] = "../data/IC5063_x3nl030/"
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infiles = ['x3nl0301r_c0f.fits','x3nl0302r_c0f.fits','x3nl0303r_c0f.fits']
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# psf_file = 'IC5063_f502m00.fits'
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# globals()['plots_folder'] = "../plots/IC5063_x3nl030/"
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globals()['plots_folder'] = "../plots/IC5063_x3nl030/"
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# globals()['data_folder'] = "../data/NGC1068_x14w010/"
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# infiles = ['x14w0101t_c0f.fits','x14w0102t_c0f.fits','x14w0103t_c0f.fits',
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@@ -122,10 +122,10 @@ def main():
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crop = False #Crop to desired ROI
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final_display = False
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# Polarization map output
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figname = 'NGC1068_FOC' #target/intrument name
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figname = 'IC5063_FOC' #target/intrument name
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figtype = '_combine_FWHM020' #additionnal informations
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SNRp_cut = 5. #P measurments with SNR>3
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SNRi_cut = 50. #I measurments with SNR>30, which implies an uncertainty in P of 4.7%.
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SNRp_cut = 3. #P measurments with SNR>3
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SNRi_cut = 60. #I measurments with SNR>30, which implies an uncertainty in P of 4.7%.
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step_vec = 1 #plot all vectors in the array. if step_vec = 2, then every other vector will be plotted
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# if step_vec = 0 then all vectors are displayed at full length
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@@ -176,13 +176,13 @@ def main():
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# see Jedrzejewski, R.; Nota, A.; Hack, W. J., A Comparison Between FOC and WFPC2
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# Bibcode : 1995chst.conf...10J
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I_stokes, Q_stokes, U_stokes, Stokes_cov = proj_red.compute_Stokes(data_array, error_array, data_mask, headers, FWHM=smoothing_FWHM, scale=smoothing_scale, smoothing=smoothing_function)
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## Step 3:
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# Rotate images to have North up
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if rotate_stokes:
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alpha = headers[0]['orientat']
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I_stokes, Q_stokes, U_stokes, Stokes_cov, headers, data_mask = proj_red.rotate_Stokes(I_stokes, Q_stokes, U_stokes, Stokes_cov, data_mask, headers, -alpha, SNRi_cut=None)
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# Compute polarimetric parameters (polarization degree and angle).
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P, debiased_P, s_P, s_P_P, PA, s_PA, s_PA_P = proj_red.compute_pol(I_stokes, Q_stokes, U_stokes, Stokes_cov, headers)
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