Measuring extragalactic Faraday rotation
|
|
- Cassandra Brown
- 6 years ago
- Views:
Transcription
1 Measuring extragalactic Faraday rotation N. Oppermann*, H. Junklewitz*, M. Greiner*, T.A. Enßlin*, T. Akahori, E. Carretti, B.M. Gaensler, A. Goobar, L. Harvey-Smith, M. Johnston-Hollitt, L. Pratley, D.H.F.M. Schnitzeler, J.M. Stil, V. Vacca* *MPI für Astrophysik
2 Galactic Faraday rotation
3 Faraday rotation Angular Power Spectrum pr ev th iou is sw wo or rk k
4 Numerical Information Field Theory Information Field Theory Selig et al. (arxiv: ) Code &
5 Theory Applications... D3PO Selig et al. (2013) arxiv: is a versatile PYTHON library incorporating CYTHON, C++, and C libraries operates regardless of the underlying spatial grid and its resolution The Y wayway signal inference TheNIFT signal inference by Marco S 5
6 Theory Applications D3PO Grid independence The Y wayway signal inference TheNIFT signal inference by Marco S 6
7 Theory Applications D3PO Grid independence 1D 2D x128 2D 32x32 The Y wayway signal inference TheNIFT signal inference by Marco S 7
8 Theory Applications D3PO Grid independence 1D 2D x128 2D 32x32 The Y wayway signal inference TheNIFT signal inference by Marco S 8
9 Theory Applications... D3PO Selig et al. (2013) arxiv: is a versatile PYTHON library incorporating CYTHON, C++, and C libraries operates regardless of the underlying spatial grid and its resolution abstracts spaces, fields, and operators into an object-orientated framework The Y wayway signal inference TheNIFT signal inference by Marco S 9
10 Theory Applications classes object space field operator parameters domain space domain space field values target space D3PO Selig et al. (2013) arxiv: instance methods applying to fields The Y wayway signal inference TheNIFT signal inference by Marco S 10
11 Theory Applications classes object space operator field point_space rg_space lm_space hp_space gl_space nested_space D3PO Selig et al. (2013) arxiv: unstructured list of points n-dimensional regular grid spherical harmonics Gauss-Legendre grid HEALPIX grid (arbitrary product of grids) The Y wayway signal inference TheNIFT signal inference by Marco S 11
12 Theory Applications classes object space operator field point_space rg_space lm_space hp_space gl_space nested_space D3PO Selig et al. (2013) arxiv: probing diagonal_operator power_operator projection_operator vecvec_operator response_operator invertible_operator propagator_operator explicit_operator The Y wayway signal inference TheNIFT signal inference by Marco S 12
13 Spectral smoothness prior Oppermann et al. (2012) unknown signal correlations inverse-gamma prior The Y wayway signal inference TheNIFT signal inference by Marco S 13
14 Spectral smoothness prior Oppermann et al. (2012) unknown signal correlations inverse-gamma prior and spectral smoothness prior σ2 = 1000 σ2 = The Y wayway signal inference TheNIFT signal inference by Marco S 14
15 Galactic Faraday rotation
16 Data filtering
17 Data filtering
18
19
20 Faraday rotation dispersion
21 AreAllyou a VIP or a SIP? data are equal! VIP = Very Informative Point, SIP = Somewhat Informative Point
22
23
24 VIP = Very Informative Point, SIP = Somewhat Informative Point
25 Posterior samples
26 Correlation structure in posterior samples
27 Information gain on
28 Summary New method to measure extragalactic Faraday rotation statistically. Verified with simulated data. Gives an extragalactic Faraday dispersion of 6.4 rad/m² for most reasonable data split in VIP and SIP categories. Method provides a posteriori samples of individual extragalactic RMs for further studies. Although this posterior sample was drawn under a specific prior (extragalactic RM variance is uniform), simple re-weighting enables their usage under other priors as well.
NIFTY Numerical Information Field Theory
Astronomy & Astrophysics manuscript no. NIFTY c ESO 2013 June 5, 2013 NIFTY Numerical Information Field Theory a versatile PYTHON library for signal inference Marco Selig 1, Michael R. Bell 1, Henrik Junklewitz
More informationInformation Field Theory. Torsten Enßlin MPI for Astrophysics Ludwig Maximilian University Munich
Information Field Theory Torsten Enßlin MPI for Astrophysics Ludwig Maximilian University Munich Information Field Theory signal field: degrees of freedom data set: finite additional information needed
More informationRM Synthesis. & magnetic field statistics. Max-Planck-Institut für Astrophysik
A8 RM Synthesis & magnetic field statistics Torsten Enßlin, Rainer Beck, Marcus Brüggen Michael Bell, Thomas Riller, Henrik Junklewitz [Andre Waelkens, Petr Kuchar, Niels Oppermann,...] Max-Planck-Institut
More informationCosmic Magnetism. Marijke Haverkorn, on behalf of the SKA Cosmic Magnetism Science Working Group
Cosmic Magnetism Marijke Haverkorn, on behalf of the SKA Cosmic Magnetism Science Working Group The Magnetism Science Working Group Core Members: Sui Ann Mao (co-chair) George Heald (co-chair) Ivan Agudo
More informationSurveying the magnetic field of the Milky Way with SKA1
Surveying the magnetic field of the Milky Way with SKA1 Image: JPL PlanetQuest Dominic Schnitzeler (MPIfR), 23/1/2014 schnitzeler@mpifr-bonn.mpg.de Overview What are the hot topics? Which tools do we have
More informationProbing RM due to the IGMF with SKA
Probing RM due to the IGMF with SKA Takuya Akahori Kagoshima University / SKA Organization Department of Physics and Astronomy, Graduate School of Science and Engineering Japan SKA Consortium / SKA Cosmic
More informationProbing RMs due to Magnetic Fields in the Cosmic Web
Probing RMs due to Magnetic Fields in the Cosmic Web Takuya Akahori JSPS Postdoctoral Fellow for Research Abroad Sydney Institute for Astronomy, The University of Sydney Japan SKA Consortium Cosmic Magnetism
More informationWanted: The best model for the distribution of electrons in the Milky Way. Dominic Schnitzeler (MPIfR), 12/7/2012
Wanted: The best model for the distribution of electrons in the Milky Way Dominic Schnitzeler (MPIfR), 12/7/2012 schnitzeler@mpifr-bonn.mpg.de Abstract NE2001 is not the most accurate n_e model Most n_e
More informationVERY LARGE ARRAY SKY SURVEY
1 VERY LARGE ARRAY SKY SURVEY POLARIZATION (TOMOGRAPHY) Lawrence Rudnick, University of Minnesota Galactic Center (Survey) Multiwavelength Image Credit: X-ray: NASA/UMass/D.Wang et al., Radio: N RAO/AUI/NSF/NRL/N.Kassim,
More informationProbing magnetic helicity with synchrotron radiation and Faraday rotation. N. Oppermann, H. Junklewitz, G. Robbers, and T. A.
A&A 53, A89 (2) DOI:.5/4-636/25545 c ESO 2 Astronomy & Astrophysics Probing magnetic helicity with synchrotron radiation and Faraday rotation N. Oppermann, H. Junklewitz, G. Robbers, and T. A. Enßlin Max
More informationA compiled catalog of rotation measures of radio point sources
Research in Astronomy and Astrophysics RESEARCH PAPERS A compiled catalog of rotation measures of radio point sources To cite this article: Jun Xu and Jin-Lin Han 2014 Res. Astron. Astrophys. 14 942 View
More informationThe Galactic magnetic field
The Galactic magnetic field Marijke Haverkorn (Nijmegen/Leiden) ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) Big Questions: What is the origin of galactic magnetic fields?
More informationUncovering magnetic field topology from synchrotron polarization
Science at Low Frequencies III, Pasadena, 2016-12-06 Uncovering magnetic field topology from synchrotron polarization Niels Oppermann Multifrequency surveys Many existing / upcoming polarization surveys
More informationFARADAY ROTATION MEASURE SYNTHESIS OF UGC 10288, NGC 4845, NGC 3044
FARADAY ROTATION MEASURE SYNTHESIS OF UGC 10288, NGC 4845, NGC 3044 PATRICK KAMIENESKI DYLAN PARÉ KENDALL SULLIVAN PI: DANIEL WANG July 21, 2016 Madison, WI OUTLINE Overview of RM Synthesis: Benefits Basic
More informationParkes MHz Rotation Measure Survey
Parkes 300-900 MHz Rotation Measure Survey Maik Wolleben E. Carretti, J. Dickey, A. Fletcher, B. Gaensler, J. L. Han, M. Haverkorn, T. Landecker, J. Leahy, N. McClure-Griffiths, D. McConnell, W. Reich,
More informationThe Global Magneto-Ionic Medium Survey
The Global Magneto-Ionic Medium Survey The Global Magneto-Ionic Medium Survey studying the polarized emission from the Galaxy The Global Magneto-Ionic Medium Survey GMIMS studying the polarized emission
More informationDES Galaxy Clusters x Planck SZ Map. ASTR 448 Kuang Wei Nov 27
DES Galaxy Clusters x Planck SZ Map ASTR 448 Kuang Wei Nov 27 Origin of Thermal Sunyaev-Zel'dovich (tsz) Effect Inverse Compton Scattering Figure Courtesy to J. Carlstrom Observables of tsz Effect Decrease
More informationAn Angular Multigrid Acceleration Method for S n Equations with Highly Forward-Peaked Scattering
An Angular Multigrid Acceleration Method for S n Equations with Highly Forward-Peaked Scattering Bruno Turcksin & Jean C. Ragusa & Jim E. Morel Texas A&M University, Dept. of Nuclear Engineering Bruno
More informationThe gamma-ray source-count distribution as a function of energy
The gamma-ray source-count distribution as a function of energy Istituto Nazionale di Fisica Nucleare, Sezione di Torino, via P. Giuria, 1, I-10125 Torino, Italy E-mail: zechlin@to.infn.it Photon counts
More informationMagnetic Fields in the Milky Way
Magnetic Fields in the Milky Way Wolfgang Reich Max-Planck-Institut für Radioastronomie Bonn Why is the Galactic B-field of interest? highest spatial resolution of B-fields clarify its role in spiral galaxies
More informationSemantics for Probabilistic Programming
Semantics for Probabilistic Programming Chris Heunen 1 / 21 Bayes law P(A B) = P(B A) P(A) P(B) 2 / 21 Bayes law P(A B) = P(B A) P(A) P(B) Bayesian reasoning: predict future, based on model and prior evidence
More informationSAMPLING DISTRIBUTIONS
SAPLING DISTRIBUTIONS Average U.S. Height in Inches (ales; 20-29yr) Individual Values 61 62 63 64 64 65 65 66 66 66 61 64 67 69 68 69 68 69 67 68 69 67 68 69 67 68 69 67 68 69 x 71 71 71 71 71 71 71 72
More informationTypes of Spatial Data
Spatial Data Types of Spatial Data Point pattern Point referenced geostatistical Block referenced Raster / lattice / grid Vector / polygon Point Pattern Data Interested in the location of points, not their
More informationMeasuring magnetism in the Milky Way with the Square Kilometre Array
Measuring magnetism in the Milky Way with the Square Kilometre Array 1,2, Takuya Akahori 3, Ettore Carretti 4, Katia Ferrière 5, Peter Frick 6, Bryan Gaensler 3,7, George Heald 8, Melanie Johnston-Hollitt
More informationPolarised synchrotron simulations for EoR experiments
Centre for Radio Cosmology Polarised synchrotron simulations for EoR experiments The broad impact of Low Frequency Observing Bologna, 19-23 June 2017 Marta Spinelli in collaboration with M. Santos and
More informationRotation Measure Synthesis of the Local Magnetized ISM
Rotation Measure Synthesis of the Local Magnetized ISM Maik Wolleben Covington Fellow, DRAO Outline Polarization, Faraday Rotation, and Rotation Measure Synthesis The Data: GMIMS The Global Magneto Ionic
More informationStatistical Inference
Statistical Inference Classical and Bayesian Methods Class 5 AMS-UCSC Tue 24, 2012 Winter 2012. Session 1 (Class 5) AMS-132/206 Tue 24, 2012 1 / 11 Topics Topics We will talk about... 1 Confidence Intervals
More informationThe Hydrogen Atom. Thornton and Rex, Ch. 7
The Hydrogen Atom Thornton and Rex, Ch. 7 Applying Schrodinger s Eqn to the Hydrogen Atom The potential: -1 e 2 V(r) = 4p e0 r Use spherical polar coordinates (with y(x,y,z) => y(r,q,f) ): 1 y 1 y ( r
More informationCosmology & CMB. Set5: Data Analysis. Davide Maino
Cosmology & CMB Set5: Data Analysis Davide Maino Gaussian Statistics Statistical isotropy states only two-point correlation function is needed and it is related to power spectrum Θ(ˆn) = lm Θ lm Y lm (ˆn)
More informationarxiv: v2 [astro-ph.ga] 14 Dec 2018
Draft version December 17, 2018 Typeset using L A TEX manuscript style in AASTeX62 The Galactic Magneto-Ionic Medium Survey: Moments of the Faraday Spectra arxiv:1812.05399v2 [astro-ph.ga] 14 Dec 2018
More informationMore. The Zeeman Effect. Normal Zeeman Effect
More The Zeeman Effect As we mentioned in Chapter 3, the splitting of spectral lines when an atom is placed in an external magnetic field was looked for by Faraday, predicted on the basis of classical
More informationMore. The Zeeman Effect. Normal Zeeman Effect
More The Zeeman Effect As we mentioned in Chapter, the splitting of spectral lines when an atom is placed in an external magnetic field was looked for by Faraday, predicted on the basis of classical theory
More informationObservations of Magnetic Fields in Intracluster Medium. Govoni Federica INAF Osservatorio Astronomico di Cagliari
Observations of Magnetic Fields in Intracluster Medium Govoni Federica INAF Osservatorio Astronomico di Cagliari Collaborators: M. Murgia, L. Feretti, G. Giovannini, V. Vacca, A. Bonafede IAU 2012 China
More informationASKAP Commissioning Update #7 April-July Latest results from the BETA test array
ASKAP Commissioning Update #7 April-July 2014 Welcome to the seventh edition of the ASKAP Commissioning Update. This includes all the latest results from commissioning of the six-antenna Boolardy Engineering
More informationStudy of Large-Scale Galactic Magnetic Fields at Low Frequencies. Jana Köhler - MPIfR -
Study of Large-Scale Galactic Magnetic Fields at Low Frequencies Jana Köhler - MPIfR - How to measure Magnetic Fields??? How to measure Galactic Magnetic Field? Linear Polarization of Starlight product
More informationUnravelling the origin of large-scale magnetic fields in galaxy clusters and beyond through Faraday Rotation Measures with the SKA
Unravelling the origin of large-scale magnetic fields in galaxy clusters and beyond through Faraday Rotation Measures with the SKA 1 Franco Vazza 1, Marcus Brüggen 1, Takuya Akahori 2, Ettore Carretti
More informationInferring source polarisation properties from SKA observations. Joern Geisbuesch
Inferring source polarisation properties from SKA observations In collaboration with Paul Alexander, Rosie Bolton, Martin Krause April 2008 University of Cambridge Department of Physics Motivation and
More informationMulti-frequency polarimetry of a complete sample of faint PACO sources. INAF-IRA (Bologna)
Multi-frequency polarimetry of a complete sample of faint PACO sources. Vincenzo Galluzzi Marcella Massardi DiFA (University of Bologna) INAF-IRA (Bologna) INAF-IRA & Italian ARC The state-of-the-art The
More informationPoS(AASKA14)041. Three-dimensional Tomography of the Galactic and Extragalactic Magnetoionic Medium with the SKA
Three-dimensional Tomography of the Galactic and Extragalactic Magnetoionic Medium with the SKA 1, W. van Straten 2, T. J. W. Lazio 3, A. Deller 4, C. Sobey 4, J. Xu 1, D. Schnitzeler 5, H. Imai 6, S.
More informationA Case for Development of the UWL Receiver for Parkes
Dick Manchester 4 December 2013 A Case for Development of the UWL Receiver for Parkes CSIRO ASTRONOMY AND SPACE SCIENCE The Parkes UWL Receiver Design Goals Received band: 0.7 4.0 GHz Wideband single-pixel
More informationTurbulence in geodynamo simulations
Turbulence in geodynamo simulations Nathanaël Schaeffer, A. Fournier, D. Jault, J. Aubert, H-C. Nataf,... ISTerre / CNRS / Université Grenoble Alpes Journée des utilisateurs CIMENT, Grenoble, 23 June 2016
More informationS-PASS and Giant Magnetised outflows from the Centre of the Milky Way
S-PASS and Giant Magnetised outflows from the Centre of the Milky Way Ettore Carretti The Universe as seen by Planck Noordwijk - 4 April 2013 CSIRO ASTRONOMY AND SPACE SCIENCE Outline S-PASS: S-band Polarization
More informationquantization condition.
/8/016 PHYS 34 Modern Physics Atom II: Hydrogen Atom Roadmap for Exploring Hydrogen Atom Today Contents: a) Schrodinger Equation for Hydrogen Atom b) Angular Momentum in Quantum Mechanics c) Quantum Number
More informationBayesian Inference for the Multivariate Normal
Bayesian Inference for the Multivariate Normal Will Penny Wellcome Trust Centre for Neuroimaging, University College, London WC1N 3BG, UK. November 28, 2014 Abstract Bayesian inference for the multivariate
More informationSolutions for Assignment of Week 06 Introduction to Astroparticle Physics
s for Assignment of Week 06 Introduction to Astroparticle Physics Georg G. Raffelt Max-Planck-Institut für Physik (Werner-Heisenberg-Institut) Föhringer Ring 6, 80805 München Email: raffelt(at)mppmu.mpg.de
More informationSoma De Post-doctoral Fellow, Arizona State University presentation at 27th Texas Symposium, Dec 11,2013
Linear Polarization of CMB and 21cm & Circular Polarization of CMB Soma De Post-doctoral Fellow, Arizona State University presentation at 27th Texas Symposium, Dec 11,2013 Collaboration: Levon Pogosian
More informationnek5000 massively parallel spectral element simulations
nek5000 massively parallel spectral element simulations PRACE Scientific Seminar HPC Boosts Science, 22th February 2011 P. Schlatter & D. S. Henningson Linné Flow Centre, KTH Mechanics Fluid flows Tornado,
More informationPrediction of ESTSP Competition Time Series by Unscented Kalman Filter and RTS Smoother
Prediction of ESTSP Competition Time Series by Unscented Kalman Filter and RTS Smoother Simo Särkkä, Aki Vehtari and Jouko Lampinen Helsinki University of Technology Department of Electrical and Communications
More informationKathrin Egberts Max-Planck-Institut für Kernphysik, Heidelberg for the H.E.S.S. Collaboration
Kathrin Egberts Max-Planck-Institut für Kernphysik, Heidelberg for the H.E.S.S. Collaboration Outline The H.E.S.S. Experiment The H.E.S.S. Electron Measurement Gamma-Ray Background Hadronic Background
More informationSpatio-Temporal Models for Areal Data
Spatio-Temporal Models for Areal Data Juan C. Vivar (jcvivar@dme.ufrj.br) and Marco A. R. Ferreira (marco@im.ufrj.br) Departamento de Métodos Estatísticos - IM Universidade Federal do Rio de Janeiro (UFRJ)
More informationENVIRONMENTAL DATA ANALYSIS WILLIAM MENKE JOSHUA MENKE WITH MATLAB COPYRIGHT 2011 BY ELSEVIER, INC. ALL RIGHTS RESERVED.
ENVIRONMENTAL DATA ANALYSIS WITH MATLAB WILLIAM MENKE PROFESSOR OF EARTH AND ENVIRONMENTAL SCIENCE COLUMBIA UNIVERSITY JOSHUA MENKE SOFTWARE ENGINEER JOM ASSOCIATES COPYRIGHT 2011 BY ELSEVIER, INC. ALL
More informationT.I.H.E. IT 233 Statistics and Probability: Sem. 1: 2013 ESTIMATION AND HYPOTHESIS TESTING OF TWO POPULATIONS
ESTIMATION AND HYPOTHESIS TESTING OF TWO POPULATIONS In our work on hypothesis testing, we used the value of a sample statistic to challenge an accepted value of a population parameter. We focused only
More informationFast Radio Burst Dispersion Measures & Rotation Measures
Keith Vanderlinde; NASA Fast Radio Burst Dispersion Measures & Rotation Measures Bryan Gaensler! (University of Toronto)!! with Tony Piro, Klaus Dolag,! Anthony Walters,! Amanda Weltman, Yin-Zhe Ma,! Manisha
More informationJVLA Wideband Polarimetry Observations on a Sample of High Rotation Measure Sources
galaxies Article JVLA Wideband Polarimetry Observations on a Sample of High Rotation Measure Sources Alice Pasetto 1, *, Carlos Carrasco-González 2, Gabriele Bruni 1, Aritra Basu 1, Shane O Sullivan 3,
More informationDNS STUDY OF TURBULENT HEAT TRANSFER IN A SPANWISE ROTATING SQUARE DUCT
10 th International Symposium on Turbulence and Shear Flow Phenomena (TSFP10), Chicago, USA, July, 2017 DNS STUDY OF TURBULENT HEAT TRANSFER IN A SPANWISE ROTATING SQUARE DUCT Bing-Chen Wang Department
More informationData Mining Chapter 4: Data Analysis and Uncertainty Fall 2011 Ming Li Department of Computer Science and Technology Nanjing University
Data Mining Chapter 4: Data Analysis and Uncertainty Fall 2011 Ming Li Department of Computer Science and Technology Nanjing University Why uncertainty? Why should data mining care about uncertainty? We
More informationarxiv: v1 [astro-ph.ga] 29 Oct 2012
Draft version September 10, 2018 Preprint typeset using L A TEX style emulateapj v. 5/2/11 THE GALACTIC MAGNETIC FIELD Ronnie Jansson and Glennys R. Farrar Center for Cosmology and Particle Physics, Department
More informationarxiv: v1 [astro-ph.ga] 20 Oct 2017
Draft version October 23, 2017 Preprint typeset using L A TEX style emulateapj v. 12/16/11 ADVANCED DIAGNOSTICS FOR THE STUDY OF LINEARLY POLARIZED EMISSION. I: DERIVATION C. A. Herron 1, B. M. Gaensler
More informationarxiv: v2 [astro-ph] 17 Dec 2007
Astronomy & Astrophysics manuscript no. ms October 27, 216 (DOI: will be inserted by hand later) arxiv:711.417v2 [astro-ph] 17 Dec 27 The Distance of the SNR Kes 75 and PWN PSR J1846-258 System D.A. Leahy
More informationp(x ω i 0.4 ω 2 ω
p( ω i ). ω.3.. 9 3 FIGURE.. Hypothetical class-conditional probability density functions show the probability density of measuring a particular feature value given the pattern is in category ω i.if represents
More informationCLUMPY: A public code for γ-ray and ν signals from dark matter structures.
CLUMPY: A public code for γ-ray and ν signals from dark matter structures. Moritz Hütten, DESY Zeuthen for the CLUMPY developers: Vincent Bonnivard, Moritz Hütten, Emmanuel Nezri, Aldée Charbonnier, Céline
More informationKey Science Project on. Cosmic Magnetism. Rainer Beck, MPIfR
Key Science Project on Cosmic Magnetism Rainer Beck, MPIfR LOFAR Key Science Projects Epoch of re-ionization Groningen Extragalactic surveys Leiden Transients and pulsars Amsterdam/Manchester Cosmic rays
More informationDead Layer and Active Volume Determination for GERDA Phase II
Dead Layer and Active Volume Determination for GERDA Phase II Björn Lehnert on behalf of the GERDA Collaboration DPG Spring Meeting 05/02/2013 Dresden Institut für Kern- und Teilchenphysik Dead Layer (DL)
More informationOptimization of the Wavelet analysis to search for point sources of cosmic-rays
Optimization of the Wavelet analysis to search for point sources of cosmic-rays von Ania Koob Bachelorarbeit in Physik vorgelegt der Fakultät für Mathematik, Informatik und Naturwissenschaften der Rheinisch-Westfälischen
More informationarxiv:astro-ph/ v1 10 Nov 1999
Pulsar Astronomy 2000 and Beyond ASP Conference Series, Vol. e iπ + 1, 2000 M. Kramer, N. Wex, and R. Wielebinski, eds. The Parkes Multibeam Pulsar Survey arxiv:astro-ph/9911185v1 10 Nov 1999 F. Camilo
More informationThe Magnetized Interstellar Medium
The Magnetized Interstellar Medium Proceedings of the conference 8 12 September 2003 Sheraton Voyager Hotel Antalya, Turkey Editors Bülent Uyanıker, Wolfgang Reich, Richard Wielebinski Organized by Max-Planck-Institut
More informationMFM Practitioner Module: Risk & Asset Allocation. John Dodson. February 3, 2010
MFM Practitioner Module: Risk & Asset Allocation Estimator February 3, 2010 Estimator Estimator In estimation we do not endow the sample with a characterization; rather, we endow the parameters with a
More informationAppendix: Nomenclature
Appendix: Nomenclature 209 Appendix: Nomenclature Chapter 2: Roman letters A amplitude of surface wave m A j (complex) amplitude of tidal component [various] a right ascension rad or a magnitude of tidal
More informationNonstationary spatial process modeling Part II Paul D. Sampson --- Catherine Calder Univ of Washington --- Ohio State University
Nonstationary spatial process modeling Part II Paul D. Sampson --- Catherine Calder Univ of Washington --- Ohio State University this presentation derived from that presented at the Pan-American Advanced
More informationSearches for cosmic ray anisotropies at ultra-high energies
Searches for cosmic ray anisotropies at ultra-high energies Haris Lyberis*, on behalf the Pierre Auger Collaboration * U n i v e r s i t é P a r i s V I I D e n i s d i d e r o t, P a r i s, F r a n c
More informationChapter 10: Unresolved Stellar Populations
Chapter 10: Unresolved Stellar Populations We now consider the case when individual stars are not resolved. So we need to use photometric and spectroscopic observations of integrated magnitudes, colors
More informationSpectral Elements. Introduction recalling the elastic wave equation
Spectral Elements Introduction recalling the elastic wave equation The spectral-element method: General concept domain mapping from space-continuous to space-discrete time extrapolation Gauss-Lobatto-Legendre
More informationGRACE Gravity Model GGM02
GRACE Gravity Model GGM02 The GGM02S gravity model was estimated with 363 days (spanning April 2002 through December 2003) of GRACE K-band range-rate, attitude, and accelerometer data. No Kaula constraint,
More informationKneib, Fahrmeir: Supplement to "Structured additive regression for categorical space-time data: A mixed model approach"
Kneib, Fahrmeir: Supplement to "Structured additive regression for categorical space-time data: A mixed model approach" Sonderforschungsbereich 386, Paper 43 (25) Online unter: http://epub.ub.uni-muenchen.de/
More informationThe Nonhydrostatic Unified Model of the Atmosphere (NUMA): CG Dynamical Core
The Nonhydrostatic Unified Model of the Atmosphere (NUMA): CG Dynamical Core Frank Giraldo Department of Applied Mathematics Naval Postgraduate School Monterey CA 93943 http://faculty.nps.edu/projects/numa
More information2D Image Processing. Bayes filter implementation: Kalman filter
2D Image Processing Bayes filter implementation: Kalman filter Prof. Didier Stricker Kaiserlautern University http://ags.cs.uni-kl.de/ DFKI Deutsches Forschungszentrum für Künstliche Intelligenz http://av.dfki.de
More informationParallel Particle Filter in Julia
Parallel Particle Filter in Julia Gustavo Goretkin December 12, 2011 1 / 27 First a disclaimer The project in a sentence. workings 2 / 27 First a disclaimer First a disclaimer The project in a sentence.
More informationBayesian SAE using Complex Survey Data Lecture 4A: Hierarchical Spatial Bayes Modeling
Bayesian SAE using Complex Survey Data Lecture 4A: Hierarchical Spatial Bayes Modeling Jon Wakefield Departments of Statistics and Biostatistics University of Washington 1 / 37 Lecture Content Motivation
More informationStatistical techniques for data analysis in Cosmology
Statistical techniques for data analysis in Cosmology arxiv:0712.3028; arxiv:0911.3105 Numerical recipes (the bible ) Licia Verde ICREA & ICC UB-IEEC http://icc.ub.edu/~liciaverde outline Lecture 1: Introduction
More informationGYRE: Yet another oscillation code, why we need it and how it works
GYRE: Yet another oscillation code, why we need it and how it works Rich Townsend & Seth Teitler University of Wisconsin-Madison What might one want from a new code? Improved flexibility to handle new
More informationImproved Astronomical Inferences via Nonparametric Density Estimation
Improved Astronomical Inferences via Nonparametric Density Estimation Chad M. Schafer, InCA Group www.incagroup.org Department of Statistics Carnegie Mellon University Work Supported by NSF, NASA-AISR
More informationAnalysis of the modulation in the first harmonic of the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
Analysis of the modulation in the first harmonic of the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory H. Lyberis 1 for the Pierre Auger Collaboration 2 1 Université
More informationAccuracy and transferability of GAP models for tungsten
Accuracy and transferability of GAP models for tungsten Wojciech J. Szlachta Albert P. Bartók Gábor Csányi Engineering Laboratory University of Cambridge 5 November 214 Motivation Number of atoms 1 1 2
More informationCHAPTER 17 CHI-SQUARE AND OTHER NONPARAMETRIC TESTS FROM: PAGANO, R. R. (2007)
FROM: PAGANO, R. R. (007) I. INTRODUCTION: DISTINCTION BETWEEN PARAMETRIC AND NON-PARAMETRIC TESTS Statistical inference tests are often classified as to whether they are parametric or nonparametric Parameter
More information1. (3) Write Gauss Law in differential form. Explain the physical meaning.
Electrodynamics I Midterm Exam - Part A - Closed Book KSU 204/0/23 Name Instructions: Use SI units. Where appropriate, define all variables or symbols you use, in words. Try to tell about the physics involved,
More informationWeb Appendix for Hierarchical Adaptive Regression Kernels for Regression with Functional Predictors by D. B. Woodard, C. Crainiceanu, and D.
Web Appendix for Hierarchical Adaptive Regression Kernels for Regression with Functional Predictors by D. B. Woodard, C. Crainiceanu, and D. Ruppert A. EMPIRICAL ESTIMATE OF THE KERNEL MIXTURE Here we
More informationOn random sequence spacing distributions
On random sequence spacing distributions C.T.J. Dodson School of Mathematics, Manchester University Manchester M6 1QD, UK ctdodson@manchester.ac.uk Abstract The random model for allocation of an amino
More informationThe Canadian Initiative for Radio Astronomy Data Analysis
The Canadian Initiative for Radio Astronomy Data Analysis Bryan Gaensler (University of Toronto) with Erik Rosolowsky, Stefi Baum, Vicky Kaspi, Chris O Dea, Ue-Li Pen, Kris Sigurdson, Greg Sivakoff, Kristine
More informationElectromagnetic Modeling and Simulation
Electromagnetic Modeling and Simulation Erin Bela and Erik Hortsch Department of Mathematics Research Experiences for Undergraduates April 7, 2011 Bela and Hortsch (OSU) EM REU 2010 1 / 45 Maxwell s Equations
More informationSTRUCTURE IN THE ROTATION MEASURE SKY
Accepted for publication in The Astrophysical Journal Preprint typeset using L A TEX style emulateapj v. 11/26/04 STRUCTURE IN THE ROTATION MEASURE SKY J. M. Stil, A. R. Taylor, and C. Sunstrum Institute
More informationReport from the last MKSP polarization imaging busy week, November 4-6
Report from the last MKSP polarization imaging busy week, November 4-6 H. Junklewitz 1, M. Brentjens, A. Clarke, J. Farnes, G. Heald, V. Heesen, D. Mulcahy, C. Riseley, S. Sridhar on behalf of the LOFAR
More informationDynamical modelling of galaxies. Eugene Vasiliev
Dynamical modelling of galaxies Eugene Vasiliev DAGAL summer school, Marseille, 2014 Plan Overview of dynamical modelling problem Theoretical and observational approaches The Schwarzschild orbit superposition
More informationCMB Lensing Reconstruction on PLANCK simulated data
CMB Lensing Reconstruction on PLANCK simulated data L. Perotto, J. Bobin, S. Plaszczynski, J.-L. Starck, A. Lavabre Laurence Perotto - LAL Orsay ADA V, may 7-9 Outlines CMB lensing as a cosmological tools
More informationParticle Physics Beyond Laboratory Energies
Particle Physics Beyond Laboratory Energies Francis Halzen Wisconsin IceCube Particle Astrophysics Center Nature s accelerators have delivered the highest energy protons, photons and neutrinos closing
More informationExperimental Design and Data Analysis for Biologists
Experimental Design and Data Analysis for Biologists Gerry P. Quinn Monash University Michael J. Keough University of Melbourne CAMBRIDGE UNIVERSITY PRESS Contents Preface page xv I I Introduction 1 1.1
More informationVLBA Imaging of the Blazar, J
VLBA Imaging of the Blazar, J08053+6144 Daniel Zirzow Jeffrey Karle Joe Craig May 11, 2009 Contents 1 Introduction 2 2 Calibration of VLBA Data 3 3 Imaging J08053+6144 at 5 GHz & 15 GHz 4 4 Model Fitting
More informationLinear and Nonlinear Models
Erik W. Grafarend Linear and Nonlinear Models Fixed Effects, Random Effects, and Mixed Models magic triangle 1 fixed effects 2 random effects 3 crror-in-variables model W DE G Walter de Gruyter Berlin
More informationTAKEOVER TIME IN PARALLEL POPULATIONS WITH MIGRATION
TAKEOVER TIME IN PARALLEL POPULATIONS WITH MIGRATION Günter Rudolph Universität Dortmund Fachbereich Informatik Lehrstuhl für Algorithm Engineering 441 Dortmund / Germany Guenter.Rudolph@uni-dortmund.de
More informationSKA AND THE COSMOLOGICAL EVOLUTION OF CLUSTER MAGNETIC FIELDS
SKA AND THE COSMOLOGICAL EVOLUTION OF CLUSTER MAGNETIC FIELDS MARTIN KRAUSE UNIVERSITY OF CAMBRIDGE, UNIVERSITÄTSSTERNWARTE MÜNCHEN & MAX-PLANCK-INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK COLLABORATORS: PAUL
More informationThe local dark matter halo density. Riccardo Catena. Institut für Theoretische Physik, Heidelberg
The local dark matter halo density Riccardo Catena Institut für Theoretische Physik, Heidelberg 17.05.2010 R. Catena and P. Ullio, arxiv:0907.0018 [astro-ph.co]. To be published in JCAP Riccardo Catena
More information