Exemple #1
0
 def get_psf_errors(self, kernel, sigma_bkg, star_list):
     """
     returns a error map of sigma prop Intensity for a stacked psf estimation
     :param psf_kwargs:
     :param star_list:
     :return:
     """
     psf_size = len(kernel)
     kernel_mean = util.image2array(kernel)
     weights = np.zeros(len(star_list))
     cov_i = np.zeros((psf_size**2, psf_size**2))
     num_stars = len(star_list)
     for i in range(0, num_stars):
         star_list_i = star_list[i].copy()
         star = util.cut_edges(star_list_i, psf_size)
         weights[i] = np.sum(star)
         rel_array = np.array(
             [util.image2array(star) / weights[i] - kernel_mean])
         a = (rel_array.T).dot(rel_array)
         cov_i += a
     factor = 1. / (num_stars)
     #weights_sum = sum(weights)
     sigma2_stack = factor * util.array2image(np.diag(cov_i))
     psf_stack = copy.deepcopy(kernel)
     sigma2_stack_new = sigma2_stack  # - (data_kwargs['sigma_background']**2/weights_sum)
     sigma2_stack_new[np.where(sigma2_stack_new < 0)] = 0
     psf_stack[np.where(psf_stack < sigma_bkg)] = sigma_bkg
     error_map = sigma2_stack_new / (psf_stack)**2
     #error_map[np.where(error_map < psf_stack**2/data_kwargs['reduced_noise'])] = 0
     # n = len(error_map)
     #error_map[(n-1)/2-1:(n-1)/2+2,(n-1)/2-1:(n-1)/2+2] += 0
     #error_map = filters.gaussian_filter(error_map, sigma=0.5)
     return error_map
Exemple #2
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 def __init__(self,
              image,
              sigma,
              poisson,
              sampling_option,
              deltaPix=1,
              mask=None,
              subgrid_res=1,
              x_grid=None,
              y_grid=None):
     """
     initializes all the classes needed for the chain
     """
     self.image = util.image2array(image)
     self.numPix = len(image)
     self.deltaPix = deltaPix
     self.subgrid_res = subgrid_res
     self.background = sigma
     self.poisson = poisson
     if x_grid is None or y_grid is None:
         self.x_grid, self.y_grid = util.make_grid(self.numPix, deltaPix,
                                                   subgrid_res)
     else:
         self.x_grid, self.y_grid = util.make_subgrid(
             x_grid, y_grid, subgrid_res)
     self.gaussian = Gaussian()
     self.moffat = Moffat()
     self.sampling_option = sampling_option
     if not mask is None:
         self.mask = util.image2array(mask)
     else:
         self.mask = np.ones((self.numPix, self.numPix))
Exemple #3
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    def plot_pixel_histogram(self, image):
        imgh = util.image2array(image)

        # print some statistics about the image
        print('Image minimum = ', min(imgh))
        print('Image maximum = ', max(imgh))
        print('Image mean = ', np.mean(imgh))
        print('Image standard deviation = ', np.std(imgh))

        # now plot a histogram of the image values
        plt.figure(2)
        plt.hist(imgh, bins=100, histtype='stepfilled')

        plt.show()  # display the plots

        plow = -1.
        phi = 1.
        q = np.where((imgh >= plow) & (imgh <= phi))
        imghcut = imgh[q]

        print('Image minimum = ', min(imghcut))
        print('Image maximum = ', max(imghcut))
        print('Image mean = ', np.mean(imghcut))
        print('Image standard deviation = ', np.std(imghcut))

        return 0
 def get_coordinates(self, x_min, x_max, y_min, y_max, wcs):
     """
     :param xc: center in ra
     :param yc: center in dec
     :param x_min: min pixel x-axis
     :param x_max: max pixel x-axis
     :param y_min: min pixel y-axis
     :param y_max: max pixel y-axis
     :param wcs: coordinate class initialized with the fits file of the original image
     :return: ra_coord, dec_coord in units of arc seconds centered to the cutout position
     """
     x_coords = np.linspace(x_min, x_max - 1, x_max - x_min)
     y_coords = np.linspace(y_min, y_max - 1, y_max - y_min)
     x_coords, y_coords = np.meshgrid(x_coords, y_coords)
     ra_coords, dec_coords = wcs.all_pix2world(x_coords, y_coords, 0)
     ra_coords -= self.ra
     dec_coords -= self.dec
     ra_coords *= 3600
     dec_coords *= 3600
     ra_coords = util.image2array(ra_coords)
     dec_coords = util.image2array(dec_coords)
     return ra_coords, dec_coords
Exemple #5
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if len(data) > 300:
    factor = 2
    if len(data) % factor != 0:
        res = len(data) % factor
        data_g = data[:-res, :-res]
        data = rebin.block(data_g,
                           (len(data_g) / factor, len(data_g) / factor),
                           factor=factor)
    else:
        data = rebin.block(data, (len(data) / factor, len(data) / factor),
                           factor=factor)

x, y = util.make_grid(numPix=len(data), deltapix=1)  # make a coordinate grid

image_1d = util.image2array(data)  # map 2d image in 1d data array

n_max = 100  # choice of number of shapelet basis functions, 150 is a high resolution number, but takes long
beta = len(data) / 20.  # shapelet scale parameter
# return the shapelet coefficients
param_list = shapeletSet.decomposition(image_1d,
                                       x,
                                       y,
                                       n_max,
                                       beta,
                                       1.,
                                       center_x=0,
                                       center_y=0)
# reconstruct M31 with the shapelet coefficients
image_reconstructed = shapeletSet.function(x,
                                           y,