コード例 #1
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def test_model_image(imsize, nproc, count, chunk=8):
    psf = None
    model_orig = create_model()
    imfit = Imfit(model_orig,
                  psf=psf,
                  quiet=True,
                  nproc=nproc,
                  chunk_size=chunk)
    shape = (imsize, imsize)
    imfit.getModelImage(shape)
    t1 = time.time()
    imfit._modelObject._testCreateModelImage(count)
    return time.time() - t1
コード例 #2
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ファイル: mock_galaxy.py プロジェクト: streeto/SpecMorph
def fit_spectra(full_spectra, full_noise, flux_unit, init_model):
    PSF = moffat_psf(fwhm=2.4, size=9)
    fitter = Imfit(init_model, PSF, quiet=True)
    models = []
    for i in xrange(0, full_spectra.shape[-1]):
#         print '#'*50, i
        f__l = full_spectra[..., i] / flux_unit
        err__l = full_noise[..., i] / flux_unit
        fitter.fit(f__l, err__l)
        if fitter.nValidPixels < 1000:
            print '(%d) Too many masked pixels.' % i
        if fitter.nPegged < 0:
            print '(%d) Pegged parameters.' % i
        m = fitter.getModelDescription()
#         print m.bulge.I_e.value, m.bulge.r_e.value, m.disk.I_0.value, m.disk.h.value
        models.append(m)
    return models
コード例 #3
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ファイル: fitting.py プロジェクト: streeto/SpecMorph
def fit_image(flux, noise, guess_model, PSF=None,
              mode='LM', insist=False, quiet=True, nproc=None, use_cash_statistics=False):
    '''
    Doc me!
    '''
    imfit = Imfit(guess_model, PSF, quiet=quiet, nproc=nproc)
    imfit.fit(flux, noise,
              mode=mode,
              error_type='sigma',
              use_cash_statistics=(mode != 'LM' and use_cash_statistics))
    logger.debug('Valid pix: %d | Iter.: %d | pegged: %d | fit stat.: %f | BIC: %f' % \
                 (imfit.nValidPixels, imfit.nIter, imfit.nPegged, imfit.reducedFitStatistic, imfit.BIC))
    fitted_model = imfit.getModelDescription()
    logger.debug('     Fitted model:\n%s\n\n' % str(fitted_model))
    if not imfit.fitConverged or imfit.nPegged > 0:
        logger.warn('Bad fit: did not converge or pegged parameter.')
        if mode == 'LM' and insist:
            logger.warn('     Retrying using N-M simplex.')
            imfit.fit(flux, noise,
                      mode='NM',
                      error_type='sigma',
                      use_cash_statistics=use_cash_statistics)
            fitted_model = imfit.getModelDescription()
            if imfit.fitConverged:
                logger.debug('     N-M simplex fit statistic: %f | BIC: %f' % (imfit.reducedFitStatistic, imfit.BIC))
            else:
                logger.warn('     Bad fit: N-M simplex did not converge.')
                logger.debug('     Fitted model:\n%s\n\n' % str(fitted_model))
    return fitted_model, imfit.fitConverged, imfit.reducedFitStatistic
コード例 #4
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ファイル: test_imfit.py プロジェクト: streeto/python-imfit
def test_fitting():
    psf = gaussian_psf(2.5, size=9)
    model_orig = create_model()
    imfit = Imfit(model_orig, psf=psf, quiet=False)

    noise_level = 0.1
    shape = (100, 100)
    image = imfit.getModelImage(shape)
    noise = image * noise_level
    image += (np.random.random(shape) * noise)
    mask = np.zeros_like(image, dtype='bool')
    
    imfit.fit(image, noise, mask)
    model_fitted = imfit.getModelDescription()

    orig_params = get_model_param_array(model_orig)
    fitted_params = get_model_param_array(model_fitted)

    assert_allclose(orig_params, fitted_params, rtol=noise_level)
コード例 #5
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ファイル: mock_galaxy.py プロジェクト: streeto/SpecMorph
def get_images(db):
    K = fitsQ3DataCube(db, smooth=False)
    mask = ~K.qMask
    qSignal = np.ma.array(K.qSignal, mask=mask)
    qNoise = np.ma.array(K.qNoise, mask=mask)
    
#     PA, ba = K.getEllipseParams()
    
    model = galaxy_model(K.x0, K.y0, bulge=True, disk=True,
                         I_e=1, r_e=12, n=1.5, PA_b=90.0, ell_b=0.5,
                         I_0=1, h=12, PA_d=90, ell_d=0.5)
    PSF = moffat_psf(fwhm=2.4, size=9)
    fitter = Imfit(model, PSF, quiet=True)
    fitter.fit(qSignal, qNoise)
    model_image = fitter.getModelImage()
    model = fitter.getModelDescription()
    bulge_image, disk_image = create_model_images(qSignal.shape, PSF, model)
    bulge_image = np.ma.array(bulge_image, mask=mask)
    disk_image = np.ma.array(disk_image, mask=mask)
    bulge_frac = bulge_image / model_image
    disk_frac = disk_image / model_image
    bulge_noise = np.sqrt(bulge_frac) * qNoise
    disk_noise = np.sqrt(disk_frac) * qNoise
    return model, qSignal, qNoise, model_image, bulge_image, bulge_noise, disk_image, disk_noise
コード例 #6
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ファイル: test_imfit.py プロジェクト: perwin/python-imfit
def test_fitting():
    psf = gaussian_psf(2.5, size=9)
    model_orig = create_model()
    imfit = Imfit(model_orig, psf=psf, quiet=False)

    noise_level = 0.1
    shape = (100, 100)
    image = imfit.getModelImage(shape)
    noise = image * noise_level
    image += (np.random.random(shape) * noise)
    mask = np.zeros_like(image, dtype='bool')

    imfit.fit(image, noise, mask)
    model_fitted = imfit.getModelDescription()

    orig_params = get_model_param_array(model_orig)
    fitted_params = get_model_param_array(model_fitted)

    assert_allclose(orig_params, fitted_params, rtol=noise_level)
コード例 #7
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ファイル: psf_calib_g.py プロジェクト: streeto/SpecMorph
model.x0.setLimitsRel(5, 5)
model.y0.setValue(flux[0].shape[0] / 2)
model.y0.setLimitsRel(5, 5)
model.addFunction(psf_func)

print 'Initial PSF model:'
print model
good = []
chi2 = []
flag = []
fitmodel = []
modelflux = []
for i, f in enumerate(flux):
    star = path.basename(cubes[i])
    print 'Fitting PSF %d of %d (%s)' % (i, len(flux), star)
    imfit = Imfit(model, quiet=True)
    imfit.fit(f, mode='NM', use_model_for_errors=False, use_cash_statistics=False)
    _goodfraction = float(imfit.nValidPixels) / float(f.size)
    print '    Good pixels: %.1f %%' % (_goodfraction  * 100)
    good.append(_goodfraction)
    print '    Fit converged? %s' % imfit.fitConverged
    flag.append(not imfit.fitConverged)
    print '    Fit statistic: %f' % imfit.fitStatistic
    chi2.append(imfit.fitStatistic)

    _fitmodel = imfit.getModelDescription()
    fitmodel.append(_fitmodel)
    model_f = imfit.getModelImage()
    modelflux.append(model_f)

    imradius = 10
コード例 #8
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ファイル: plot_models.py プロジェクト: streeto/SpecMorph
def rad_prof(model, bins):
    imfit = Imfit(model, quiet=False)
    image = imfit.getModelImage((model.y0.value * 2, model.x0.value * 2))
    return radialProfile(image, bins, x0, y0, pa=0.0, ba=1.0)
コード例 #9
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ファイル: mock_galaxy.py プロジェクト: streeto/SpecMorph
def create_image(shape, PSF, model):
    imfit = Imfit(model, PSF, quiet=True)
    image = imfit.getModelImage(shape)
    return image
コード例 #10
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ファイル: fitting.py プロジェクト: streeto/SpecMorph
def model_image(model, shape, PSF=None, nproc=None):
    imfit = Imfit(model, PSF, quiet=True, nproc=nproc)
    return imfit.getModelImage(shape)
コード例 #11
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ファイル: psf.py プロジェクト: streeto/SpecMorph
model.y0.setLimitsRel(3, 3)
model.addFunction(psf_func)

print 'Initial PSF model:'
print model

psfmodels = []
psfflags = []
goodfraction = []
chi2 = []
for i in xrange(psfflux.shape[0]):
    wl = psf_wl[i]
    pf = psfflux[i] - psfbg[i]
    pf[pf <= 0] = np.ma.masked
    print 'Fitting PSF %d of %d (%s \AA)' % (i, fill_flux.shape[0], wl)
    imfit = Imfit(model, quiet=True)
    imfit.fit(pf, mode='NM', use_model_for_errors=False)
    _goodfraction = float(imfit.nValidPixels) / float(psfflux[i].size)
    goodfraction.append(_goodfraction)
    flagged = not imfit.fitConverged or _goodfraction < 0.5
    psfflags.append(flagged)
    print '    Fit statistic: %f' % imfit.fitStatistic
    print '    Reduced fit statistic: %f' % imfit.reducedFitStatistic
    print '    Valid pix: %.1f %%' % (_goodfraction * 100.0)
    print '    Flagged? %s' % flagged
    chi2.append(imfit.fitStatistic)
    fitmodel = imfit.getModelDescription()
    modelimage = imfit.getModelImage()
    psfmodels.append(fitmodel)
    print fitmodel