示例#1
0
def transfer_to_result_ps(data,
                          ps_result,
                          image_ps,
                          image_host,
                          error_map,
                          filt,
                          fixcenter,
                          ID,
                          cut=0,
                          plot_compare=True,
                          QSO_msk_list="",
                          pix_sz='drz06',
                          QSO_msk=None,
                          tag=None):
    #==============================================================================
    # Translate the e1, e2 to phi_G and q
    #==============================================================================
    #==============================================================================
    # Save the result
    #==============================================================================
    from roundme import roundme
    result = {}
    ##==============================================================================
    ##Plot the images for adopting in the paper
    ##==============================================================================
    from flux_profile import total_compare
    data = data
    QSO = image_ps
    if QSO_msk is None:
        QSO_mask = data * 0 + 1
    else:
        QSO_mask = QSO_msk
    if len(image_host) == 0:
        host = data * 0
        label = ['data', 'QSO', 'host=0', 'model', 'normalized residual']
    elif len(image_host) > 0:
        host = np.zeros_like(image_host[0])
        for i in range(len(image_host)):
            host += image_host[i]
        label = [
            'data', 'QSO', '{0}objs'.format(i), 'model', 'normalized residual'
        ]  #Print the numbers of objects
    flux_list = [data, QSO, host, error_map]
    import glob
    mask_list = glob.glob(QSO_msk_list)  # Read *.reg files in a list.
    #    print "mask_list,muhahah", mask_list
    fig = total_compare(label_list=label,
                        flux_list=flux_list,
                        target_ID=ID,
                        pix_sz=pix_sz,
                        data_mask_list=mask_list,
                        data_cut=cut,
                        zp=zp,
                        plot_compare=plot_compare,
                        msk_image=QSO_mask)
    if tag is not None:
        fig.savefig("{0}_SB_profile.pdf".format(tag), bbox_inches='tight')
    # =============================================================================
    # Calculate reduced Chisq and save to result
    # =============================================================================
    chiq_map = ((data - image_ps - host) / (error_map))**2 * QSO_mask
    pixels = len(error_map)**2 - (1 - QSO_mask).sum()
    reduced_Chisq = chiq_map.sum() / pixels
    result = roundme(result)
    result['redu_Chisq'] = round(reduced_Chisq, 6)
    return result
for i in range(len(chain_list)):
    f, axes = chain_plot.plot_chain_list(chain_list,i)
    plt.show()

agn_image = pyfits.getdata('./allscience/l{0}_{1}_cutout.fits'.format(ID,fr))
if len(image_host) == 1:
    host = image_host[0]
    label = ['data', 'QSO', 'host', 'model', 'normalized residual']
elif len(image_host) >1:
    host = np.zeros_like(image_host[0])
    for i in range(len(image_host)):
        host += image_host[i]
    label = ['data', 'QSO', 'host as {0} components'.format(i+1), 'model', 'normalized residual']  #Print the numbers
        
flux_list = [agn_image, image_ps[0], host, error_map]
fig = total_compare(label_list = label, flux_list = flux_list, target_ID = ID, pix_sz=pix_sz, zp = zp,
                    plot_compare = False, msk_image = QSO_msk)
from IPython.display import display
display(fig)


#%% Recover the plot
from lenstronomy.Plots.model_plot import ModelPlot
modelPlot = ModelPlot(multi_band_list, kwargs_model, kwargs_result,
                          arrow_size=0.02, cmap_string="gist_heat", likelihood_mask_list=[QSO_msk])
f, axes = plt.subplots(3, 3, figsize=(16, 16), sharex=False, sharey=False)
modelPlot.data_plot(ax=axes[0,0], text="Data")
modelPlot.model_plot(ax=axes[0,1])
modelPlot.normalized_residual_plot(ax=axes[0,2], v_min=-6, v_max=6)
modelPlot.decomposition_plot(ax=axes[1,0], text='Host galaxy', source_add=True, unconvolved=True)
modelPlot.decomposition_plot(ax=axes[1,1], text='Host galaxy convolved', source_add=True)
modelPlot.decomposition_plot(ax=axes[1,2], text='All components convolved', source_add=True, lens_light_add=True, point_source_add=True)
示例#3
0
def transfer_to_result(data,
                       source_result,
                       ps_result,
                       image_ps,
                       image_host,
                       error_map,
                       zp,
                       fixcenter,
                       ID,
                       cut=0,
                       plot_compare=True,
                       QSO_msk_list="",
                       pix_sz=0.168,
                       QSO_msk=None,
                       tag=None):
    #==============================================================================
    # Translate the e1, e2 to phi_G and q
    #==============================================================================
    import lenstronomy.Util.param_util as param_util
    source_result[0]['phi_G'], source_result[0][
        'q'] = param_util.ellipticity2phi_q(source_result[0]['e1'],
                                            source_result[0]['e2'])

    #==============================================================================
    # Save the result
    #==============================================================================
    from roundme import roundme
    import copy
    result = copy.deepcopy(source_result[0])
    del result['e1']
    del result['e2']
    result['QSO_amp'] = ps_result[0]['point_amp'][0]
    result['host_amp'] = image_host[0].sum()
    result['host_flux_ratio_percent'] = result['host_amp'] / (
        result['QSO_amp'] + result['host_amp']) * 100
    zp = zp
    result['host_mag'] = -2.5 * np.log10(result['host_amp']) + zp
    #print "The host flux is ~:", image_host.sum()/(image_ps.sum() + image_host.sum())
    # =============================================================================
    # Save QSO position to result if not fix center
    # =============================================================================
    if fixcenter == False:
        result['qso_x'] = ps_result[0]['ra_image'][0]
        result['qso_y'] = ps_result[0]['dec_image'][0]

    ##==============================================================================
    ##Plot the images for adopting in the paper
    ##==============================================================================
    from flux_profile import total_compare
    data = data
    QSO = image_ps
    if QSO_msk is None:
        QSO_mask = data * 0 + 1
    else:
        QSO_mask = QSO_msk
    if len(image_host) == 1:
        host = image_host[0]
        label = ['data', 'QSO', 'host', 'model', 'normalized residual']
    elif len(image_host) > 1:
        host = np.zeros_like(image_host[0])
        for i in range(len(image_host)):
            host += image_host[i]
        label = [
            'data', 'QSO', 'host+{0}objs'.format(i), 'model',
            'normalized residual'
        ]  #Print the numbers of objects
    flux_list = [data, QSO, host, error_map]
    import glob
    mask_list = glob.glob(QSO_msk_list)  # Read *.reg files in a list.
    #    print "mask_list,muhahah", mask_list
    fig = total_compare(label_list=label,
                        flux_list=flux_list,
                        target_ID=ID,
                        pix_sz=pix_sz,
                        data_mask_list=mask_list,
                        data_cut=cut,
                        zp=zp,
                        plot_compare=plot_compare,
                        msk_image=QSO_mask)
    if tag is not None:
        fig.savefig("{0}_SB_profile.pdf".format(tag), bbox_inches='tight')
    fig1 = total_compare(label_list=label,
                         flux_list=flux_list,
                         target_ID=ID,
                         pix_sz=pix_sz,
                         data_mask_list=mask_list,
                         data_cut=cut,
                         zp=zp,
                         plot_compare=plot_compare,
                         msk_image=QSO_mask,
                         if_annuli=True)
    if tag is not None:
        fig1.savefig("{0}_SB_profile_annuli.pdf".format(tag),
                     bbox_inches='tight')

    # =============================================================================
    # Calculate reduced Chisq and save to result
    # =============================================================================
    chiq_map = ((data - image_ps - host) / (error_map))**2 * QSO_mask
    pixels = len(error_map)**2 - (1 - QSO_mask).sum()
    reduced_Chisq = chiq_map.sum() / pixels
    result = roundme(result)
    result['redu_Chisq'] = round(reduced_Chisq, 6)
    return result
示例#4
0
from flux_profile import total_compare
QSO_im, err_map, QSO_bkg, PSF, pix_scale, zp, qso_fr_center, fr_c_RA_DEC = gen_fit_id(
    image_folder, QSO_RA, QSO_DEC, filename, cut_frame=120, subbkl=sub_bkg)
ct = (len(QSO_im) -
      len(image_host[0])) / 2  # If want to cut to 61, QSO_im[ct:-ct,ct:-ct]

if len(image_host) == 1:
    host = image_host[0]
    label = ['data', 'QSO', 'host', 'model', 'normalized residual']
elif len(image_host) > 1:
    host = np.zeros_like(image_host[0])
    for i in range(len(image_host)):
        host += image_host[i]
    label = [
        'data', 'QSO', 'host as {0} components'.format(i + 1), 'model',
        'normalized residual'
    ]  #Print the numbers of objects
agn_image = QSO_im[ct:-ct, ct:-ct]
error_map = err_map[ct:-ct, ct:-ct]
flux_list = [agn_image, image_ps, host, error_map]

total_compare(label_list=label,
              flux_list=flux_list,
              target_ID=QSO_id + '-' + band,
              pix_sz=pix_scale,
              zp=zp,
              plot_compare=False,
              msk_image=np.ones_like(agn_image))

#fig.savefig("{0}_SB_profile.pdf".format(name_save), bbox_inches = 'tight')