コード例 #1
0
ファイル: compute_sdss_pca.py プロジェクト: zyq11223/astroML
def spec_iterative_pca(outfile, n_ev=10, n_iter=20, norm='L2'):
    """
    This function takes the file outputted above, performs an iterative
    PCA to fill in the gaps, and appends the results to the same file.
    """
    data_in = np.load(outfile)
    spectra = data_in['spectra']
    mask = data_in['mask']

    res = iterative_pca(spectra,
                        mask,
                        n_ev=n_ev,
                        n_iter=n_iter,
                        norm=norm,
                        full_output=True)

    input_dict = {key: data_in[key] for key in data_in.files}

    # don't save the reconstructed spectrum: this can easily
    # be recomputed from the other parameters.
    input_dict['mu'] = res[1]
    input_dict['evecs'] = res[2]
    input_dict['evals'] = res[3]
    input_dict['norms'] = res[4]
    input_dict['coeffs'] = res[5]

    np.savez(outfile, **input_dict)
コード例 #2
0
ファイル: compute_sdss_pca.py プロジェクト: BTY2684/astroML
def spec_iterative_pca(outfile, n_ev=10, n_iter=20, norm='L2'):
    """
    This function takes the file outputted above, performs an iterative
    PCA to fill in the gaps, and appends the results to the same file.
    """
    data_in = np.load(outfile)
    spectra = data_in['spectra']
    mask = data_in['mask']

    res = iterative_pca(spectra, mask,
                        n_ev=n_ev, n_iter=n_iter, norm=norm,
                        full_output=True)

    input_dict = dict([(key, data_in[key]) for key in data_in.files])

    # don't save the reconstructed spectrum: this can easily
    # be recomputed from the other parameters.
    input_dict['mu'] = res[1]
    input_dict['evecs'] = res[2]
    input_dict['evals'] = res[3]
    input_dict['norms'] = res[4]
    input_dict['coeffs'] = res[5]

    np.savez(outfile,
             **input_dict)
コード例 #3
0
ファイル: test_iterative_PCA.py プロジェクト: BTY2684/astroML
def test_iterative_PCA(n_samples=50, n_features=40):
    np.random.seed(0)

    # construct some data that is well-approximated
    #  by two principal components
    x = np.linspace(0, np.pi, n_features)
    x0 = np.linspace(0, np.pi, n_samples)
    X = np.sin(x) * np.cos(0.5 * (x - x0[:, None]))

    # mask 10% of the pixels
    M = (np.random.random(X.shape) > 0.9)

    # reconstruct and check accuracy
    for norm in (None, 'L1', 'L2'):
        X_recons = iterative_pca(X, M, n_ev=2, n_iter=10, norm=norm)

        assert_array_almost_equal(X, X_recons, decimal=2)
コード例 #4
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def eigenspectra(data, output='spectra', wvrange=(6600,9000)):
    # data is a fits table (or similar) 2d array

    notnan = (data.LBIN[0] > wvrange[0]) & (data.LBIN[0] < wvrange[1])
    N = len(data)
    n = len(data.LBIN[0][notnan])

    smooth=True
    spectra = np.empty((N,n))
    mask = np.empty((N,n))
    for i in range(N):
        flx = data.SPECCALIB[i][notnan]
        wv = data.LBIN[i][notnan]

        if smooth:
            spec = Spectrum(wv,flx)
            spec.smooth(width='5', filtertype='gaussian', replace=True)
            flx = spec.flux
            wv = spec.x
        
        spectra[i,:] = flx
        mask[i,:] = (~np.isfinite(flx)) | (flx == 0)

    x_recon, mu, evecs, evals, norms, coeffs = iterative_pca(spectra, mask, n_ev=8, n_iter=15, norm='L2', full_output=True)
    evals_cs = (evals**2).cumsum()
    evals_cs /= evals_cs[-1]

    spec_mean = x_recon.mean(0)

    coeffs = np.empty((N,N))
    for i, spec in enumerate(x_recon):
        cfs = np.dot(evecs, spec/norms[i] - mu)
        coeffs[:,i] = cfs

    if output == 'spectra':
        return x_recon, norms, notnan, mask
    elif output == 'components':
        return evecs, evals, coeffs