musecube_old.py 文件源码

def __init__(self, filename_cube, filename_white=None, pixelsize=0.2 * u.arcsec, n_fig=1,
                 flux_units=1E-20 * u.erg / u.s / u.cm ** 2 / u.angstrom, vmin=None, vmax=None, wave_cal='air'):
        """
        Parameters
        ----------
        filename_cube: string
            Name of the MUSE datacube .fits file
        filename_white: string
            Name of the MUSE white image .fits file
        pixel_size : float or Quantity, optional
            Pixel size of the datacube, if float it assumes arcsecs.
            Default is 0.2 arcsec
        n_fig : int, optional
            XXXXXXXX
        flux_units : Quantity
            XXXXXXXXXX

        """

        # init
        self.color = False
        self.cmap = ""
        self.flux_units = flux_units
        self.n = n_fig
        plt.close(self.n)
        self.wave_cal = wave_cal


        self.filename = filename_cube
        self.filename_white = filename_white
        self.load_data()
        self.white_data = fits.open(self.filename_white)[1].data
        self.hdulist_white = fits.open(self.filename_white)
        self.white_data = np.where(self.white_data < 0, 0, self.white_data)

        if not vmin:
            self.vmin=np.nanpercentile(self.white_data,0.25)
        else:
            self.vmin = vmin
        if not vmax:
            self.vmax=np.nanpercentile(self.white_data,98.)
        else:
            self.vmax = vmax
        self.gc2 = aplpy.FITSFigure(self.filename_white, figure=plt.figure(self.n))
        self.gc2.show_grayscale(vmin=self.vmin, vmax=self.vmax)

        # self.gc = aplpy.FITSFigure(self.filename, slices=[1], figure=plt.figure(20))
        self.pixelsize = pixelsize
        gc.enable()
        # plt.close(20)
        print("MuseCube: Ready!")