172,343 research outputs found

    Calculation of Critical Values for Somerville's FDR Procedures

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    A Fortran 95 program has been written to calculate critical values for the step-up and step-down FDR procedures developed by Somerville (2004). The program allows for arbitrary selection of number of hypotheses, FDR rate, one- or two-sided hypotheses, common correlation coefficient of the test statistics and degrees of freedom. An MCV (minimum critical value) may be specified, or the program will calculate a specified number of critical values or steps in an FDR procedure. The program can also be used to efficiently ascertain an upper bound to the number of hypotheses which the procedure will reject, given either the values of the test statistics, or their p values. Limiting the number of steps in an FDR procedure can be used to control the number or proportion of false discoveries (Somerville and Hemmelmann 2007). Using the program to calculate the largest critical values makes possible efficient use of the FDR procedures for very large numbers of hypotheses.

    Somerville, H C, VX51757

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    This record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/418373Surname: SOMERVILLE. Given Name(s) or Initials: H C. Military Service Number or Last Known Location: VX51757. Missing, Wounded and Prisoner of War Enquiry Card Index Number: 30966.241879 Item: [2016.0049.50634] "Somerville, H C, VX51757

    Port Argostoli

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    surveyed by lieutenant C. H. Simpson, r.n. assisted by lieut. J. C. Tancred & L. D. Penfold and sub-lieut. H. G. C. Somerville & E. A. Constable, r.n

    Somerville, Matthew C.

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    Voice Compression and Communications: Principles and Applications for Fixes and Wireless Channels

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    Up-to-date, expert coverage of topics in wireless voice communications Voice communication is the most important facet of mobile radio service. Even when the predicted surge of wireless data and Internet services becomes a reality, voice will remain the most natural means of human communication. Voice Compression and Communications details issues in wireless voice communications and treats compression, channel coding, and wireless transmission as a joint subject. Part I covers background material, whereas Part II provides detailed information on both proprietary and standardized analysis-by-synthesis codecs, including the speech codecs of virtually all existing wireline-based and wireless systems. Parts III and IV discuss mainly research-based wideband, audio, as well as very low-rate schemes likely to find their way into future standards. Voice Compression and Communications describes fundamental concepts in a non-mathematical way early in the book for those with only a background knowledge of signal processing and communications. More advanced readers will find detailed discussions of theoretical principles, future concepts, and solutions to various specific wireless voice communications problems

    Galaxy far-infrared spectral energy distribution templates from Safarzadeh, Hayward, Ferguson & Somerville 2016 (arXiv:1509.00034)

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    This dataset contains the data and code released with Safarzadeh, Hayward, Ferguson & Somerville, 2016, ApJ, in press (http://adsabs.harvard.edu/abs/2015arXiv150900034S). In this work, we presented a set of two-parameter galaxy far-infrared spectral energy distribution (SED) templates. The templates are parameterized in terms of the IR luminosity and dust mass. They were derived from mock SEDs of simulated isolated disk galaxies and galaxy mergers, which were generated by performing radiative transfer on hydrodynamical simulations in post-processing

    Galaxy far-infrared spectral energy distribution templates from Safarzadeh, Hayward, Ferguson & Somerville 2016 (arXiv:1509.00034)

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    This dataset contains the data and code released with Safarzadeh, Hayward, Ferguson & Somerville, 2016, ApJ, in press (http://adsabs.harvard.edu/abs/2015arXiv150900034S). In this work, we presented a set of two-parameter galaxy far-infrared spectral energy distribution (SED) templates. The templates are parameterized in terms of the IR luminosity and dust mass. They were derived from mock SEDs of simulated isolated disk galaxies and galaxy mergers, which were generated by performing radiative transfer on hydrodynamical simulations in post-processing
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