add correction factor for all polarizer filters to have same transmission efficiency

This commit is contained in:
Tibeuleu
2022-10-25 11:17:50 +02:00
parent 23d802cabb
commit 700cc7e4df
15 changed files with 24 additions and 15 deletions

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@@ -49,7 +49,9 @@ for d in [data_S, data_K]:
d['SNRi'] = np.zeros(d['I'].shape)
d['SNRi'][d['sI']>0.] = d['I'][d['sI']>0.]/d['sI'][d['sI']>0.]
d['mask'] = np.logical_and(d['SNRi']>30,d['SNRp']>5)
data_S['mask'], data_K['mask'] = np.logical_and(data_S['mask'],data_K['mask']), np.logical_and(data_S['mask'],data_K['mask'])
for d in [data_S, data_K]:
d['X'], d['Y'] = np.meshgrid(np.arange(d['I'].shape[1]), np.arange(d['I'].shape[0]))
d['xy_U'], d['xy_V'] = np.where(d['mask'],d['P']*np.cos(np.pi/2.+d['PA']*np.pi/180.), np.nan), np.where(d['mask'],d['P']*np.sin(np.pi/2.+d['PA']*np.pi/180.), np.nan)
@@ -60,7 +62,6 @@ quiv0 = ax.quiver(data_S['X'],data_S['Y'],data_S['xy_U'],data_S['xy_V'],units='x
quiv1 = ax.quiver(data_K['X'],data_K['Y'],data_K['xy_U'],data_K['xy_V'],units='xy',angles='uv',scale=0.5,scale_units='xy',pivot='mid',headwidth=0.,headlength=0.,headaxislength=0.,width=0.1,color='r',alpha=0.75, label="PA through Kishimoto's pipeline")
ax.set_title(r"$SNR_P \geq 5 \; & \; SNR_I \geq 30$")
fig.legend()
plt.show()
#compute integrated polarization parameters on a specific cut
for d in [data_S, data_K]:
@@ -79,8 +80,12 @@ print('From my pipeline :\n', "P = {0:.2f} ± {1:.2f} %\n".format(data_S['P_dil'
print("From Kishimoto's pipeline :\n", "P = {0:.2f} ± {1:.2f} %\n".format(data_K['P_dil']*100.,data_K['sP_dil']*100.), "PA = {0:.2f} ± {1:.2f} °".format(data_K['PA_dil'],data_K['sPA_dil']))
#compare different types of error
print("My pipeline : average sI/I={0:.2f} ; sQ/Q={1:.2f} ; sU/U={2:.2f} ; sP/P={3:.2f}".format(np.mean(data_S['sI'][data_S['mask']]/data_S['I'][data_S['mask']]),np.mean(np.abs(data_S['sQ'][data_S['mask']]/data_S['Q'][data_S['mask']])),np.mean(np.abs(data_S['sU'][data_S['mask']]/data_S['U'][data_S['mask']])),np.mean(data_S['sP'][data_S['mask']]/data_S['P'][data_S['mask']])))
print("Kishimoto's pipeline : average sI/I={0:.2f} ; sQ/Q={1:.2f} ; sU/U={2:.2f} ; sP/P={3:.2f}".format(np.mean(data_K['sI'][data_K['mask']]/data_K['I'][data_K['mask']]),np.mean(np.abs(data_K['sQ'][data_K['mask']]/data_K['Q'][data_K['mask']])),np.mean(np.abs(data_K['sU'][data_K['mask']]/data_K['U'][data_K['mask']])),np.mean(data_K['sP'][data_K['mask']]/data_K['P'][data_K['mask']])))
xx, yy = np.indices(data_S['mask'].shape)
mask_ind = np.array([[y,x] for y,x in zip(yy[data_S['mask']],xx[data_S['mask']])])
index = mask_ind[np.random.randint(len(mask_ind))]
print("My pipeline : sI/I={0:.2f} ; sQ/Q={1:.2f} ; sU/U={2:.2f} ; sP/P={3:.2f}".format(np.mean(data_S['sI'][index[0],index[1]]/data_S['I'][index[0],index[1]]),np.mean(data_S['sQ'][index[0],index[1]]/data_S['Q'][index[0],index[1]]),np.mean(data_S['sU'][index[0],index[1]]/data_S['U'][index[0],index[1]]),np.mean(data_S['sP'][index[0],index[1]]/data_S['P'][index[0],index[1]])))
print("Kishimoto's pipeline : sI/I={0:.2f} ; sQ/Q={1:.2f} ; sU/U={2:.2f} ; sP/P={3:.2f}".format(np.mean(data_K['sI'][index[0],index[1]]/data_K['I'][index[0],index[1]]),np.mean(data_K['sQ'][index[0],index[1]]/data_K['Q'][index[0],index[1]]),np.mean(data_K['sU'][index[0],index[1]]/data_K['U'][index[0],index[1]]),np.mean(data_K['sP'][index[0],index[1]]/data_K['P'][index[0],index[1]])))
print("For random pixel in cut at {}".format(index))
for d,i in zip(['I','Q','U','P','PA','sI','sQ','sU','sP','sPA'],[0,1,2,5,8,(3,0,0),(3,1,1),(3,2,2),6,9]):
data_K[d] = np.loadtxt(path_join(root_dir_K,d+'.txt'))
with fits.open(path_join(root_dir_data_S,'NGC1068_K_FOC_bin10px.fits')) as f:
@@ -94,3 +99,5 @@ for d,i in zip(['I','Q','U','P','PA','sI','sQ','sU','sP','sPA'],[0,1,2,5,8,(3,0,
#from Kishimoto's pipeline : IQU_dir, IQU_shift, IQU_stat, IQU_trans
#from my pipeline : raw_bg, raw_flat, raw_psf, raw_shift, raw_wav, IQU_dir
# but errors from my pipeline are propagated all along, how to compare then ?
plt.show()

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@@ -509,11 +509,11 @@ def get_error(data_array, headers, error_array=None, data_mask=None,
background[i] = sub_image.sum()
if (data_array[i] < 0.).any():
print(data_array[i])
if i==0:
np.savetxt("output/s_bg.txt",error_bkg[i])
np.savetxt("output/s_wav.txt",err_wav)
np.savetxt("output/s_psf.txt",err_psf)
np.savetxt("output/s_flat.txt",err_flat)
#if i==0:
#np.savetext("output/s_bg.txt",error_bkg[i])
#np.savetext("output/s_wav.txt",err_wav)
#np.savetext("output/s_psf.txt",err_psf)
#np.savetext("output/s_flat.txt",err_flat)
if display:
plt.rcParams.update({'font.size': 10})
@@ -843,8 +843,8 @@ def align_data(data_array, headers, error_array=None, upsample_factor=1.,
#sum quadratically the errors
rescaled_error[i] = np.sqrt(rescaled_error[i]**2 + error_shift**2)
if i==1:
np.savetxt("output/s_shift.txt",error_shift)
#if i==1:
#np.savetext("output/s_shift.txt",error_shift)
shifts.append(shift)
errors.append(error)
@@ -1204,12 +1204,14 @@ def compute_Stokes(data_array, error_array, data_mask, headers,
transmit3 = np.min([trans3[header['filtnam3'].lower()] for header in headers])
transmit4 = np.min([trans4[header['filtnam4'].lower()] for header in headers])
transmit *= transmit2*transmit3*transmit4
pol_eff = np.array([pol_efficiency['pol0'], pol_efficiency['pol60'], pol_efficiency['pol120']])
#Calculating correction factor
corr = np.array([1.0*h['photflam']/h['exptime'] for h in pol_headers])*pol_headers[0]['exptime']/pol_headers[0]['photflam']
# Orientation and error for each polarizer
fmax = np.finfo(np.float64).max
pol_flux = np.array([pol0, pol60, pol120])
pol_flux = np.array([corr[0]*pol0, corr[1]*pol60, corr[2]*pol120])
coeff_stokes = np.zeros((3,3))
# Coefficients linking each polarizer flux to each Stokes parameter
@@ -1255,9 +1257,9 @@ def compute_Stokes(data_array, error_array, data_mask, headers,
s_I2_axis = np.sum([dI_dtheta[i]**2 * sigma_theta[i]**2 for i in range(len(sigma_theta))],axis=0)
s_Q2_axis = np.sum([dQ_dtheta[i]**2 * sigma_theta[i]**2 for i in range(len(sigma_theta))],axis=0)
s_U2_axis = np.sum([dU_dtheta[i]**2 * sigma_theta[i]**2 for i in range(len(sigma_theta))],axis=0)
np.savetxt("output/sI_dir.txt", np.sqrt(s_I2_axis))
np.savetxt("output/sQ_dir.txt", np.sqrt(s_Q2_axis))
np.savetxt("output/sU_dir.txt", np.sqrt(s_U2_axis))
#np.savetext("output/sI_dir.txt", np.sqrt(s_I2_axis))
#np.savetext("output/sQ_dir.txt", np.sqrt(s_Q2_axis))
#np.savetext("output/sU_dir.txt", np.sqrt(s_U2_axis))
# Add quadratically the uncertainty to the Stokes covariance matrix
Stokes_cov[0,0] += s_I2_axis