Beispiel #1
0
def _lanczos_interpolate(L, ixi, iyi, dx, dy, laccs, limages,
                         table=True):
    '''
    L: int, Lanczos order
    ixi: int, 1-d numpy array, len n, x coord in input images
    iyi:     ----""----        y
    dx: float, 1-d numpy array, len n, fractional x coord
    dy:      ----""----                    y
    laccs: list of [float, 1-d numpy array, len n]: outputs
    limages list of [float, 2-d numpy array, shape h,w]: inputs
    '''
    from miscutils import lanczos_filter
    lfunc = lanczos_filter
    if L == 3:
        try:
            from util import lanczos3_filter, lanczos3_filter_table
            # 0: no rangecheck
            if table:
                #lfunc = lambda nil,x,y: lanczos3_filter_table(x,y, 0)
                lfunc = lambda nil,x,y: lanczos3_filter_table(x,y, 1)
            else:
                lfunc = lambda nil,x,y: lanczos3_filter(x,y)
        except:
            pass

    h,w = limages[0].shape
    n = len(ixi)
    # sum of lanczos terms
    fsum = np.zeros(n)
    off = np.arange(-L, L+1)
    #fx = np.zeros(n)
    #fy = np.zeros(n)
    fx = np.zeros(n, np.float32)
    fy = np.zeros(n, np.float32)
    for oy in off:
        #print 'dy range:', min(-oy + dy), max(-oy + dy)
        lfunc(L, -oy + dy, fy)
        for ox in off:
            lfunc(L, -ox + dx, fx)
            #print 'dx range:', min(-ox + dx), max(-ox + dx)
            for lacc,im in zip(laccs, limages):
                lacc += fx * fy * im[np.clip(iyi + oy, 0, h-1),
                                     np.clip(ixi + ox, 0, w-1)]
                fsum += fx*fy
    for lacc in laccs:
        lacc /= fsum
Beispiel #2
0
def _lanczos_interpolate(L, ixi, iyi, dx, dy, laccs, limages,
                         table=True):
    '''
    L: int, Lanczos order
    ixi: int, 1-d numpy array, len n, x coord in input images
    iyi:     ----""----        y
    dx: float, 1-d numpy array, len n, fractional x coord
    dy:      ----""----                    y
    laccs: list of [float, 1-d numpy array, len n]: outputs
    limages list of [float, 2-d numpy array, shape h,w]: inputs
    '''
    from miscutils import lanczos_filter
    lfunc = lanczos_filter
    if L == 3:
        try:
            from util import lanczos3_filter, lanczos3_filter_table
            # 0: no rangecheck
            if table:
                #lfunc = lambda nil,x,y: lanczos3_filter_table(x,y, 0)
                lfunc = lambda nil,x,y: lanczos3_filter_table(x,y, 1)
            else:
                lfunc = lambda nil,x,y: lanczos3_filter(x,y)
        except:
            pass

    h,w = limages[0].shape
    n = len(ixi)
    # sum of lanczos terms
    fsum = np.zeros(n)
    off = np.arange(-L, L+1)
    #fx = np.zeros(n)
    #fy = np.zeros(n)
    fx = np.zeros(n, np.float32)
    fy = np.zeros(n, np.float32)
    for oy in off:
        #print 'dy range:', min(-oy + dy), max(-oy + dy)
        lfunc(L, -oy + dy, fy)
        for ox in off:
            lfunc(L, -ox + dx, fx)
            #print 'dx range:', min(-ox + dx), max(-ox + dx)
            for lacc,im in zip(laccs, limages):
                lacc += fx * fy * im[np.clip(iyi + oy, 0, h-1),
                                     np.clip(ixi + ox, 0, w-1)]
                fsum += fx*fy
    for lacc in laccs:
        lacc /= fsum
Beispiel #3
0
    from astrometry.util.util import lanczos3_filter, lanczos3_filter_table
    # x = np.linspace(-4, 4, 500)
    # L = np.zeros_like(x)
    # L2 = np.zeros(len(x), np.float32)
    # lanczos3_filter(x, L)
    # lanczos3_filter_table(x.astype(np.float32), L2, 1)
    # plt.clf()
    # plt.plot(x, L, 'r-')
    # plt.plot(x, L2, 'b-')
    # plt.savefig('l1.png')

    x = np.linspace(-3.5, 4.5, 8192).astype(np.float32)
    L1 = np.zeros_like(x)
    L2 = np.zeros_like(x)
    lanczos3_filter(x, L1)
    lanczos3_filter_table(x, L2, 1)
    print 'L2 - L1 RMS:', np.sqrt(np.mean((L2-L1)**2))
    
    if True:
        ra,dec = 0.,0.,
        pixscale = 1e-3
        W,H = 10,1

        cowcs = Tan(ra, dec, (W+1)/2., (H+1)/2.,
                    -pixscale, 0., 0., pixscale, W, H)
        dx,dy = 0.25, 0.
        wcs = Tan(ra, dec, (W+1)/2. + dx, (H+1)/2. + dy,
                  -pixscale, 0., 0., pixscale, W, H)

        pix = np.zeros((H,W), np.float32)
Beispiel #4
0
    from astrometry.util.util import lanczos3_filter, lanczos3_filter_table
    # x = np.linspace(-4, 4, 500)
    # L = np.zeros_like(x)
    # L2 = np.zeros(len(x), np.float32)
    # lanczos3_filter(x, L)
    # lanczos3_filter_table(x.astype(np.float32), L2, 1)
    # plt.clf()
    # plt.plot(x, L, 'r-')
    # plt.plot(x, L2, 'b-')
    # plt.savefig('l1.png')

    x = np.linspace(-3.5, 4.5, 8192).astype(np.float32)
    L1 = np.zeros_like(x)
    L2 = np.zeros_like(x)
    lanczos3_filter(x, L1)
    lanczos3_filter_table(x, L2, 1)
    print 'L2 - L1 RMS:', np.sqrt(np.mean((L2 - L1)**2))

    if True:
        ra, dec = 0., 0.,
        pixscale = 1e-3
        W, H = 10, 1

        cowcs = Tan(ra, dec, (W + 1) / 2., (H + 1) / 2., -pixscale, 0., 0.,
                    pixscale, W, H)
        dx, dy = 0.25, 0.
        wcs = Tan(ra, dec, (W + 1) / 2. + dx, (H + 1) / 2. + dy, -pixscale, 0.,
                  0., pixscale, W, H)

        pix = np.zeros((H, W), np.float32)