fix background substraction and clean repo
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@@ -19,26 +19,25 @@ 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'] = ['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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#psf_file = 'IC5063_f502m00.fits'
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globals()['plots_folder'] = "../plots/IC5063_x3nl030/"
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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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##psf_file = 'IC5063_f502m00.fits'
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#globals()['plots_folder'] = "../plots/IC5063_x3nl030/"
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#globals()['data_folder'] = "../data/NGC1068_x14w010/"
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#globals()['infiles'] = ['x14w0101t_c0f.fits','x14w0102t_c0f.fits','x14w0103t_c0f.fits',
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# 'x14w0104t_c0f.fits','x14w0105p_c0f.fits','x14w0106t_c0f.fits']
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#globals()['plots_folder'] = "../plots/NGC1068_x14w010/"
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#globals()['data_folder'] = "../data/3C405_x136060/"
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#globals()['infiles'] = ['x1360601t_c0f.fits','x1360602t_c0f.fits','x1360603t_c0f.fits']
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#globals()['plots_folder'] = "../plots/3C405_x136060/"
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globals()['data_folder'] = "../data/3C405_x136060/"
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globals()['infiles'] = ['x1360601t_c0f.fits','x1360602t_c0f.fits','x1360603t_c0f.fits']
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globals()['plots_folder'] = "../plots/3C405_x136060/"
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#globals()['data_folder'] = "../data/CygnusA_x43w0/"
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#globals()['infiles'] = ['x43w0101r_c0f.fits', 'x43w0102r_c0f.fits', 'x43w0103r_c0f.fits',
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@@ -146,10 +145,10 @@ def main():
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crop = False #Crop to desired ROI
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final_display = True
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# Polarization map output
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figname = 'IC5063_FOC' #target/intrument name
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figname = '3C405_FOC' #target/intrument name
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figtype = '_combine_FWHM020' #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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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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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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