reduce NGC1068 for comparison with Kishimoto's pipeline
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@@ -18,12 +18,13 @@ from astropy.wcs import WCS
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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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#globals()['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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#globals()['infiles'] = ['xn1c400.fits','xn2c400.fits','xn3c400.fits']
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globals()['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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#globals()['infiles'] = ['x3nl0301r_c0f.fits','x3nl0302r_c0f.fits','x3nl0303r_c0f.fits']
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@@ -90,13 +91,13 @@ from astropy.wcs import WCS
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#globals()['plots_folder'] = "../plots/3C273_x0u20/"
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#BEWARE: 5 observations separated by 1 year each (1995, 1996, 1997, 1998, 1999)
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globals()['data_folder'] = "../data/M87/POS1/"
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#globals()['data_folder'] = "../data/M87/POS1/"
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#globals()['infiles'] = ['x2py010ct_c0f.fits','x2py010dt_c0f.fits','x2py010et_c0f.fits','x2py010ft_c0f.fits'] #1995
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#globals()['infiles'] = ['x3be010ct_c0f.fits','x3be010dt_c0f.fits','x3be010et_c0f.fits','x3be010ft_c0f.fits'] #1996
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#globals()['infiles'] = ['x43r010km_c0f.fits','x43r010mm_c0f.fits','x43r010om_c0f.fits','x43r010rm_c0f.fits'] #1997
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#globals()['infiles'] = ['x43r110kr_c0f.fits','x43r110mr_c0f.fits','x43r110or_c0f.fits','x43r110rr_c0f.fits'] #1998
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globals()['infiles'] = ['x43r210kr_c0f.fits','x43r210mr_c0f.fits','x43r210or_c0f.fits','x43r210rr_c0f.fits'] #1999
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globals()['plots_folder'] = "../plots/M87/POS1/"
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#globals()['infiles'] = ['x43r210kr_c0f.fits','x43r210mr_c0f.fits','x43r210or_c0f.fits','x43r210rr_c0f.fits'] #1999
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#globals()['plots_folder'] = "../plots/M87/POS1/"
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#BEWARE: 5 observations separated by 1 year each (1995, 1996, 1997, 1998, 1999)
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#globals()['data_folder'] = "../data/M87/POS3/"
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@@ -128,28 +129,28 @@ def main():
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# Data binning
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rebin = True
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if rebin:
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pxsize = 0.05
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px_scale = 'arcsec' #pixel, arcsec or full
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pxsize = 10
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px_scale = 'pixel' #pixel, arcsec or full
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rebin_operation = 'sum' #sum or average
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# Alignement
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align_center = 'image' #If None will align image to image center
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display_data = False
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# Smoothing
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smoothing_function = 'combine' #gaussian_after, weighted_gaussian_after, gaussian, weighted_gaussian or combine
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smoothing_FWHM = 0.10 #If None, no smoothing is done
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smoothing_FWHM = None #If None, no smoothing is done
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smoothing_scale = 'arcsec' #pixel or arcsec
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# Rotation
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rotate_stokes = True #rotation to North convention can give erroneous results
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rotate_data = False #rotation to North convention can give erroneous results
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# Final crop
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crop = False #Crop to desired ROI
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final_display = True
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final_display = False
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# Polarization map output
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figname = 'M87_POS1_1999_FOC' #target/intrument name
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figtype = '_combine_FWHM010' #additionnal informations
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figname = 'NGC1068_K_FOC' #target/intrument name
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figtype = '_bin10px' #additionnal informations
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SNRp_cut = 3. #P measurments with SNR>3
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SNRi_cut = 30. #I measurments with SNR>30, which implies an uncertainty in P of 4.7%.
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step_vec = 0 #plot all vectors in the array. if step_vec = 2, then every other vector will be plotted
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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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##### Pipeline start
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