Parameter Method

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The Experts below are selected from a list of 564048 Experts worldwide ranked by ideXlab platform

Susumu Sato - One of the best experts on this subject based on the ideXlab platform.

D Scott - One of the best experts on this subject based on the ideXlab platform.

  • a comparison of the galaxy peculiar velocity field with the pscz gravity field a bayesian hyper Parameter Method
    Monthly Notices of the Royal Astronomical Society, 2012
    Co-Authors: E Branchini, D Scott
    Abstract:

    We constructed a Bayesian hyper-Parameter statistical Method to quantify the difference between predicted velocities derived from the observed galaxy distribution in the IRAS-PSCz (Point Source Catalogue Redshift) survey and peculiar velocities measured using different distance indicators. In our analysis, we find that the model–data comparison becomes unreliable beyond 70 h −1 Mpc because of the inadequate sampling by the IRAS survey of prominent, distant superclusters, like the Shapley Concentration. On the other hand, the analysis of the velocity residuals shows that the PSCz gravity field provides an adequate model to the local, ≤70 h −1 Mpc, peculiar velocity field. The hyper-Parameter combination of ENEAR, SN, A1SN and SFI++ catalogues in the Bayesian framework constrains the amplitude of the linear flow to be β = 0.53 ± 0.014. For an rms density fluctuation in the PSCz galaxy number density σ gal 8 = 0.42 ± 0.03, we obtain an estimate of the growth rate of density fluctuations f σ 8(z ∼ 0) = 0.42 ± 0.033, which is in excellent agreement with independent estimates based on different techniques.

  • a comparison of the galaxy peculiar velocity field with the pscz gravity field a bayesian hyper Parameter Method
    arXiv: Cosmology and Nongalactic Astrophysics, 2012
    Co-Authors: E Branchini, D Scott
    Abstract:

    We constructed a Bayesian hyper-Parameter statistical Method to quantify the difference between predicted velocities derived from the observed galaxy distribution in the \textit{IRAS}-PSC$z$ redshift survey and peculiar velocities measured using different distance indicators. In our analysis we find that the model--data comparison becomes unreliable beyond $70 \hmpc$ because of the inadequate sampling by \textit{IRAS} survey of prominent, distant superclusters, like the Shapley Concentration. On the other hand, the analysis of the velocity residuals show that the PSC$z$ gravity field provides an adequate model to the local, $\le 70 \hmpc$, peculiar velocity field. The hyper-Parameter combination of ENEAR, SN, A1SN and SFI++ catalogues in the Bayesian framework constrains the amplitude of the linear flow to be $\beta=0.53 \pm 0.014$. For an rms density fluctuations in the PSC$z$ galaxy number density $\sigma_8^{\rm gal}=0.42\pm0.03$, we obtain an estimate of the growth rate of density fluctuations $f\sigma_{8}(z\sim0) = 0.42 \pm 0.033$, which is in excellent agreement with independent estimates based on different techniques.

E Branchini - One of the best experts on this subject based on the ideXlab platform.

  • a comparison of the galaxy peculiar velocity field with the pscz gravity field a bayesian hyper Parameter Method
    Monthly Notices of the Royal Astronomical Society, 2012
    Co-Authors: E Branchini, D Scott
    Abstract:

    We constructed a Bayesian hyper-Parameter statistical Method to quantify the difference between predicted velocities derived from the observed galaxy distribution in the IRAS-PSCz (Point Source Catalogue Redshift) survey and peculiar velocities measured using different distance indicators. In our analysis, we find that the model–data comparison becomes unreliable beyond 70 h −1 Mpc because of the inadequate sampling by the IRAS survey of prominent, distant superclusters, like the Shapley Concentration. On the other hand, the analysis of the velocity residuals shows that the PSCz gravity field provides an adequate model to the local, ≤70 h −1 Mpc, peculiar velocity field. The hyper-Parameter combination of ENEAR, SN, A1SN and SFI++ catalogues in the Bayesian framework constrains the amplitude of the linear flow to be β = 0.53 ± 0.014. For an rms density fluctuation in the PSCz galaxy number density σ gal 8 = 0.42 ± 0.03, we obtain an estimate of the growth rate of density fluctuations f σ 8(z ∼ 0) = 0.42 ± 0.033, which is in excellent agreement with independent estimates based on different techniques.

  • a comparison of the galaxy peculiar velocity field with the pscz gravity field a bayesian hyper Parameter Method
    arXiv: Cosmology and Nongalactic Astrophysics, 2012
    Co-Authors: E Branchini, D Scott
    Abstract:

    We constructed a Bayesian hyper-Parameter statistical Method to quantify the difference between predicted velocities derived from the observed galaxy distribution in the \textit{IRAS}-PSC$z$ redshift survey and peculiar velocities measured using different distance indicators. In our analysis we find that the model--data comparison becomes unreliable beyond $70 \hmpc$ because of the inadequate sampling by \textit{IRAS} survey of prominent, distant superclusters, like the Shapley Concentration. On the other hand, the analysis of the velocity residuals show that the PSC$z$ gravity field provides an adequate model to the local, $\le 70 \hmpc$, peculiar velocity field. The hyper-Parameter combination of ENEAR, SN, A1SN and SFI++ catalogues in the Bayesian framework constrains the amplitude of the linear flow to be $\beta=0.53 \pm 0.014$. For an rms density fluctuations in the PSC$z$ galaxy number density $\sigma_8^{\rm gal}=0.42\pm0.03$, we obtain an estimate of the growth rate of density fluctuations $f\sigma_{8}(z\sim0) = 0.42 \pm 0.033$, which is in excellent agreement with independent estimates based on different techniques.

Jingfung Lin - One of the best experts on this subject based on the ideXlab platform.

  • a hybrid approach for measuring the Parameters of twisted nematic liquid crystal cells utilizing the stokes Parameter Method and a genetic algorithm
    Journal of Lightwave Technology, 2009
    Co-Authors: Weilian Lin, Jingfung Lin
    Abstract:

    A new approach is proposed for measuring the cell thickness, twist angle, pretilt angle, and azimuth angle of twisted-nematic liquid crystal (TNLC) cells utilizing the Stokes Parameter Method and a genetic algorithm (GA). In the proposed approach, the Stokes Parameters are measured for linearly polarized probe lights with polarization angles of 0deg and 45deg, respectively, with the azimuth angle of the test cell set to 0deg. The TNLC is then rotated through 45deg and the Stokes Parameters are remeasured. The four sets of Stokes Parameters are processed by GA for the data fitting to inversely derive the cell Parameters, and especially the pretilt angle is successfully obtained with slight tilt of the cell. Also, the proposed Method enables the four Parameters of the TNLC cell to be measured over the full azimuth angle range and involves a single wavelength only. Unlike existing Methods that need continuously rotating the polarizer for achieving a curve fitting in Stokes Parameters or using multiple wavelengths, this technique first proposed in this study supplies a simpler and cheaper Methodology to extract the four Parameters of TNLC cell. The experimental results show that the maximum standard deviations of the cell thickness, twist angle, pretilt angle, and azimuth angle are Deltad = 0.002 mum, Deltaphi = 0.09deg, Deltathetasp = 0.28deg, and Deltaalpha = 0.08deg, respectively. Also, the azimuth angle alpha can be extracted in the full range in this study.

Marenori Kawamura - One of the best experts on this subject based on the ideXlab platform.