예제 #1
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    def test_Sigma_dust_sync_betas_temp(self):
        NSIDE = 8
        MODEL = 'd0s0'
        INSTRUMENT = 'litebird'
        SIGNAL_TO_NOISE = 10000
        UNITS = 'uK_CMB'
        sky = pysm.Sky(get_sky(NSIDE, MODEL))
        instrument = pysm.Instrument(
            get_instrument(INSTRUMENT, NSIDE, units=UNITS))
        components = [
            cm.Dust(150., temp=20., units=UNITS),
            cm.Synchrotron(150., units=UNITS)
        ]
        ref = []
        for component in components:
            ref += component.defaults
        ref = np.array(ref)

        with suppress_stdout():
            freq_maps, noise_maps = instrument.observe(sky,
                                                       write_outputs=False)

        signal = freq_maps[:, 0, 0]  # Same signal for all the pixels
        noise = noise_maps[:, 0]
        signal_ver = signal / np.dot(signal, signal)**0.5
        noise_std = np.std([np.dot(n, signal_ver) for n in noise.T])
        maps = signal_ver * noise_std * SIGNAL_TO_NOISE
        maps = maps[:, np.newaxis] + noise

        res = basic_comp_sep(components, instrument, maps, nside=NSIDE)
        diff = (res.x.T - ref)
        postS = np.mean(diff[..., None] * diff[..., None, :], axis=0)
        S = res.Sigma.T[0]
        aac(postS, S, rtol=1. / NSIDE)
예제 #2
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    def test_Sigma_dust_one_parameter(self):
        NSIDE = 8
        MODEL = 'd0'
        INSTRUMENT = 'litebird'
        SIGNAL_TO_NOISE = 10
        sky = pysm.Sky(get_sky(NSIDE, MODEL))
        instrument = pysm.Instrument(get_instrument(INSTRUMENT, NSIDE))
        components = [cm.Dust(100., temp=20.)]
        ref = []
        for component in components:
            ref += component.defaults

        with suppress_stdout():
            freq_maps, noise_maps = instrument.observe(sky,
                                                       write_outputs=False)

        signal = freq_maps[:, 0, 0]
        noise = noise_maps[:, 0]
        signal_ver = signal / np.dot(signal, signal)**0.5
        noise_std = np.std([np.dot(n, signal_ver) for n in noise.T])
        maps = signal_ver * noise_std * SIGNAL_TO_NOISE
        maps = maps[:, np.newaxis] + noise

        res = basic_comp_sep(components,
                             instrument,
                             maps,
                             nside=hp.get_nside(maps))
        white = (res.x[0] - ref[0]) / res.Sigma[0, 0]**0.5
        _, p = kstest(white, 'norm')
        assert p > 0.01
예제 #3
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    def test_Sigma_dust_sync_betas_temp(self):
        NSIDE = 8
        MODEL = 'd0s0'
        INSTRUMENT = 'LiteBIRD'
        SIGNAL_TO_NOISE = 10000
        UNITS = 'uK_CMB'
        sky = get_sky(NSIDE, MODEL)
        instrument = get_instrument(INSTRUMENT)
        components = [
            cm.Dust(150., temp=20., units=UNITS),
            cm.Synchrotron(150., units=UNITS)
        ]
        ref = []
        for component in components:
            ref += component.defaults
        ref = np.array(ref)

        freq_maps = get_observation(instrument, sky, unit=UNITS)
        noise_maps = get_noise_realization(NSIDE, instrument, unit=UNITS)

        signal = freq_maps[:, 0, 0]  # Same signal for all the pixels
        noise = noise_maps[:, 0]
        signal_ver = signal / np.dot(signal, signal)**0.5
        noise_std = np.std([np.dot(n, signal_ver) for n in noise.T])
        maps = signal_ver * noise_std * SIGNAL_TO_NOISE
        maps = maps[:, np.newaxis] + noise
        if not hasattr(instrument, 'depth_i'):
            instrument['depth_i'] = instrument.depth_p / np.sqrt(2)

        res = basic_comp_sep(components, instrument, maps, nside=NSIDE)
        diff = (res.x.T - ref)
        postS = np.mean(diff[..., None] * diff[..., None, :], axis=0)
        S = res.Sigma.T[0]
        aac(postS, S, rtol=1. / NSIDE)
예제 #4
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    def test_Sigma_dust_one_parameter(self):
        NSIDE = 8
        MODEL = 'd0'
        INSTRUMENT = 'LiteBIRD'
        SIGNAL_TO_NOISE = 10
        sky = get_sky(NSIDE, MODEL)
        instrument = get_instrument(INSTRUMENT)
        components = [cm.Dust(100., temp=20.)]
        ref = []
        for component in components:
            ref += component.defaults

        freq_maps = get_observation(instrument, sky)
        noise_maps = get_noise_realization(NSIDE, instrument)

        signal = freq_maps[:, 0, 0]
        noise = noise_maps[:, 0]
        signal_ver = signal / np.dot(signal, signal)**0.5
        noise_std = np.std([np.dot(n, signal_ver) for n in noise.T])
        maps = signal_ver * noise_std * SIGNAL_TO_NOISE
        maps = maps[:, np.newaxis] + noise
        if not hasattr(instrument, 'depth_i'):
            instrument['depth_i'] = instrument.depth_p / np.sqrt(2)

        res = basic_comp_sep(components,
                             instrument,
                             maps,
                             nside=hp.get_nside(maps))
        white = (res.x[0] - ref[0]) / res.Sigma[0, 0]**0.5
        _, p = kstest(white, 'norm')
        assert p > 0.01
예제 #5
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    def setUp(self):
        NSIDE = 16
        MODEL = 'c1d0s0f1'
        INSTRUMENT = 'LiteBIRD'
        X0_FACTOR = 0.99
        sky = get_sky(NSIDE, MODEL)
        self.instrument = get_instrument(INSTRUMENT)
        self.freq_maps = get_observation(self.instrument, sky)

        self.components = [cm.CMB(), cm.Dust(200.), cm.Synchrotron(100.)]
        freefree = cm.PowerLaw(100.)
        freefree.defaults = [-2.14]  # Otherwise it is the same as Synchrotron
        self.components.append(freefree)
        self.input = []
        for component in self.components:
            self.input += component.defaults
            component.defaults = [d * X0_FACTOR for d in component.defaults]
예제 #6
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 def setUp(self):
     self.DX = 5e-4  # NOTE: this is a bit fine-tuned
     np.random.seed(0)
     self.n_freq = 6
     self.nu = np.logspace(1, 2.5, self.n_freq)
     self.n_stokes = 3
     self.n_pixels = 2
     self.components = [cm.CMB(), cm.Dust(200.), cm.Synchrotron(70.)]
     self.mm = MixingMatrix(*(self.components))
     self.params = [1.54, 20, -3]
     self.A = self.mm.eval(self.nu, *(self.params))
     self.A_dB = self.mm.diff(self.nu, *(self.params))
     self.A_dBdB = self.mm.diff_diff(self.nu, *(self.params))
     self.invN = uniform(size=(self.n_pixels, self.n_stokes, self.n_freq,
                               self.n_freq))
     self.invN += _T(self.invN)
     self.invN += 10 * np.eye(self.n_freq)
     self.invN *= 10
예제 #7
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    def setUp(self):
        NSIDE = 16
        MODEL = 'c1d0s0f1'
        INSTRUMENT = 'litebird'
        X0_FACTOR = 0.99
        sky = pysm.Sky(get_sky(NSIDE, MODEL))
        self.instrument = pysm.Instrument(get_instrument(INSTRUMENT, NSIDE))
        with suppress_stdout():
            self.freq_maps, self.noise = self.instrument.observe(
                sky, write_outputs=False)

        self.components = [cm.CMB(), cm.Dust(200.), cm.Synchrotron(100.)]
        freefree = cm.PowerLaw(100.)
        freefree.defaults = [-2.14]  # Otherwise it is the same as Synchrotron
        self.components.append(freefree)
        self.input = []
        for component in self.components:
            self.input += component.defaults
            component.defaults = [d * X0_FACTOR for d in component.defaults]