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Portland - EC - 570
EconometricsLecture Notes Hayashi, Chapter 3d GMM: Hypotheses TestingHypotheses Testing Suppose A.1-A.5 hold, n ( GMMW - ) d N(0,Avar( GMMW) as n. Suppose there is a consistent estimate of S (=E(gigi'). Let Est(Avar( GMMW) = (Sxz'WSxz)-1Sxz'W
Portland - EC - 570
EconometricsLecture Notes Hayashi, Chapter 1fGeneralized Least Squares Assumption 4 Revisited: E( ' |X) = Var( |X) = 2In Assumption 4 Relaxed (Assumption 4'): E( ' |X) = Var( |X) = 2V(X), with nonsingular and known V(X). OLS estimator of , b
Portland - EC - 570
EconometricsLecture Notes Hayashi, Chapter 2aConvergence: Definitions A sequence of random scalars {zn} = (z1,z2, ) converges in probability to z (a constant or a random variable) if, for any >0, limn Prob(|zn-z|> ) = 0. z is the probability lim
Portland - EC - 570
EconometricsLecture Notes Hayashi, Chapter 1aLinear Regression Notations y: Dependent Variable (Regressand) yi, i = 1,2,n X: Explanatory Variables (Regressors) xi, i = 1,2,n xij, i = 1,2,n; j = 1,2,KLinear Regression Assumption 1: Linear
Portland - EC - 570
EconometricsLecture Notes Hayashi, Chapter 1dHypothesis Testing under Normality Assumption 5: |X ~ N(0, 2In) Implications of Normality Assumption (b- )|X ~ N(0, 2(XX)-1) (bk- k)|X ~ N(0, 2([XX)-1]kk) zk ~ N(0,1) b k k zk = 2 [( X' X) 1 ]kk
Portland - EC - 570
EconometricsLecture Notes Hayashi, Chapter 2c Large Sample TheoryAssumption DGP (Data Generating Process): A stochastic process that generated the finite sample (y,X) must satisfies: Assumption 1: Linearity yi = xi' + i (i=1,2,.,n)Assumption
Portland - EC - 570
EconometricsLecture Notes Hayashi, Chapter 1bMethod-of-Moments Estimator From the implication of strict exgeneity assumption, E(xjk i) = 0 for i = 1,2,.,n and k = 1,2,.,K. That is, Moment Conditions: E(X' ) = 0 X'(y-X ) = 0 or X'y=X'X The meth
Portland - EC - 572
Year Month LEI9619590159.219590259.919590360.519590460.419590560.519590660.519590760.319590859.919590959.919591059.519591158.919591260.019600159.719600259.219600358.619600458.719600558.819600658.9
Portland - EC - 572
21.67521.71621.75621.79621.83721.87821.91821.9592222.04122.08222.12322.16422.20522.24722.28822.32922.37122.41222.45422.49622.53822.5822.62222.66422.70622.74822.7922.83322.87522.91822.9623.00323.04623.08923.13223.17
Portland - EC - 595
Year GNP Inv Price Rate 1963 596.7 90.0 0.7167 3.23 1964 637.7 97.4 0.7277 3.55 1965 691.1 113.5 0.7436 4.04 1966 756.0 125.7 0.7676 4.50 1967 799.6 122.8 0.7906 4.19 1968 873.4 133.3 0.8254 5.16 196
Portland - EC - 572
YEAR QT DPI2000 PCE20001947 1 1096.01017.21947 2 1072.81034.01947 3 1102.81037.51947 4 1089.71037.71948 1 1107.31042.61948 2 1145.31054.31948 3 1168.41056.11948 4 1171.91064.81949 1 1147.61066.11949 2 1151.410
Caltech - PH - 237
Ph 237a: Gravitational Waves6 March 2002WEEK 10: GW'S FROM NEUTRON-STAR ROTATION AND PULSATION; NUMERICAL RELATIVITY AND SIMULATIONS OF GRAVITATIONAL-WAVE SOURCES Lectures 17 by Lee Lindblom, and 18 by Mark Scheel Recommended Reading: There are n
Caltech - PH - 237
The Status and Prospects for Resonant Gravitational Wave DetectorsW.O. Hamilton Louisiana State UniversityAcknowledgements! ! ! !Odylio Aguiar Eugenio Coccia Ik Siong Heng Warren Johnson23 April 2002Albuquerque2What resonant detectors d
Caltech - PH - 237
Ph 237b: Gravitational Waves10 April 2002WEEK 12: OVERVIEW OF REAL INTERFEROMETERS; THERMAL NOISE Lecture 21 by Alan Weinstein [Real Interferometers]; Lecture 22 by Phil Willems [Thermal Noise]Recommended Reading Related to These Lectures:1.
Caltech - PH - 18
RAPID COMMUNICATIONSPHYSICAL REVIEW D, VOLUME 63, 021101 RDiscriminating a gravitational wave background from instrumental noise in the LISA detectorMassimo Tinto,* J. W. Armstrong, and F. B. EstabrookJet Propulsion Laboratory, California Insti
Caltech - PH - 237
RAPID COMMUNICATIONSPHYSICAL REVIEW D, VOLUME 63, 021101 RDiscriminating a gravitational wave background from instrumental noise in the LISA detectorMassimo Tinto,* J. W. Armstrong, and F. B. EstabrookJet Propulsion Laboratory, California Insti
Caltech - PH - 237
Physics 237b: LISA Lasers and Opticshttp:/huey.jpl.nasa.gov/~respero/lisaRobert Spero 15 May 2002Antenna size compared to signal wavelength10-18LISA-20LIGO= LLISA LIGO10= L10-2210-24 -4 -2 2 4101011010106LIGO
Caltech - PH - 13
An introduction to PoundDreverHall laser frequency stabilizationEric D. BlackLIGO Project, California Institute of Technology, Mail Code 264-33, Pasadena, California 91125Received 3 January 2000; accepted 4 April 2000 This paper is an introductio
Caltech - PH - 237
An introduction to PoundDreverHall laser frequency stabilizationEric D. BlackLIGO Project, California Institute of Technology, Mail Code 264-33, Pasadena, California 91125Received 3 January 2000; accepted 4 April 2000 This paper is an introductio
Caltech - PH - 18
THE ASTROPHYSICAL JOURNAL, 527 : 814826, 1999 December 20( 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.TIME-DELAY INTERFEROMETRY FOR SPACE-BASED GRAVITATIONAL WAVE SEARCHES J. W. ARMSTRONG, F. B. ESTABROOK, AND M
Caltech - PH - 237
THE ASTROPHYSICAL JOURNAL, 527 : 814826, 1999 December 20( 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.TIME-DELAY INTERFEROMETRY FOR SPACE-BASED GRAVITATIONAL WAVE SEARCHES J. W. ARMSTRONG, F. B. ESTABROOK, AND M
Caltech - PH - 18
Time-Delay InterferometryJohn Armstrong, Frank Estabrook, and Massimo Tinto Jet Propulsion Laboratory, California Institute of Technology Reminder of what LISA is and what the main noise sources are Why conventional laser noise cancellation metho
Caltech - PH - 237
Time-Delay InterferometryJohn Armstrong, Frank Estabrook, and Massimo Tinto Jet Propulsion Laboratory, California Institute of Technology Reminder of what LISA is and what the main noise sources are Why conventional laser noise cancellation metho
Caltech - PH - 237
Ph 237a: Gravitational Waves13 February 2002WEEK 6: PROPAGATION OF GWs THROUGH MATTER, and SLOW-MOTION APPROXIMATION FOR WAVE GENERATION Lectures 10 and 11 Recommended Reading: Some of the reading this week comes from chapter 5 of the 1989 unpubl
Caltech - PH - 237
Ph 237b: Gravitational Waves10 April 2002WEEK 13: Control Systems & Laser Locking; Interferometer Simulation & Lock Acquisition; Seismic Isolation Lecture 23 by Eric Black [Control Systems & Laser Locking]; Lecture 24, Part 1 by Matt Evans [Inter
Caltech - PH - 237
LIGOas a Large Science ProjectBarry Barish Ph237b April 23, 2002Experimental Research! Traditional Mode Single Investigator Program built around a laboratory with some equipment Experiment built to attack particular problem Support from p
Caltech - PH - 237
Ph 237a: Gravitational Waves23 January 2001WEEK 3: INTRODUCTION TO GENERAL RELATIVITY & GRAVITATIONAL WAVES Recommended Reading: 1. Blandford and Thorne, Applications of Classical Physics, [available on the web at http:/www.pma.caltech.edu/Course
Caltech - PH - 237
Ph 237b: Gravitational Waves WEEK 17: LISA Overview, and LISA's Lasers and Optics Revised version, 16 May Lecture 31 by William Folkner (JPL) [LISA Overview] Lecture 32,by Robert Spero (JPL) [LISA's Lasers and Optics]15 May 2002Reading Related to
Caltech - PH - 237
Ph 237a: Gravitational Waves WEEK 8: COMPACT BINARIES AS GW SOURCES Lectures 13 by Phinney, and 14 by Thorne & Buonanno20 February 2002Recommended Reading: As last week, there are no textbook treatments of the material covered in this week's lect
Caltech - PH - 237
Ph 237a: Gravitational Waves30 January 2002WEEK 4: WEAK GRAVITATIONAL WAVES IN OTHERWISE FLAT SPACETIME Recommended Reading: 1. Blandford and Thorne, Applications of Classical Physics, [available on the web at http:/www.pma.caltech.edu/Courses/ph
Caltech - PH - 237
Ph 237a: Gravitational Waves20 February 2002WEEK 7: ASTROPHYSICAL PHENOMENOLOGY AND BINARY STARS AS GW SOURCES Lecture 12 by Phinney Recommended Reading: There are no good textbooks or even review articles that cover all, or even most of what Phi
Caltech - PH - 237
Ph 237b: Gravitational Waves22 May 2002WEEK 18: LISA's Disturbance Reduction System and Time Delay Interferometry Lecture 33 by Bonny Schumaker (JPL) [Disturbance Reduction System] Lecture 34 by John Anderson (JPL) [Time Delay Interferometry] Rea
Caltech - PH - 237
Seismic attenuation tools for Gravitational Wave Interferometric DetectorsRiccardo DeSalvo et al. 17th of April 2002Gravitational Wave Interferometic Detector Seismic Attenuation Requirements Ground motion 10-6 ~ 10-8 m/Hz Gravitational signal
Caltech - PH - 237
Resonant Gravity Wave DetectorsW.O. Hamilton Louisiana State UniversityContributors Bruce Pipes P.S. Nayar Tom Bernat Dale Darling David Blair Jarda Kadlec Bill Oelfke Tony Mann Warren Johnson Nadja Magalhaes Martin McHugh Ik Siong He
Caltech - PH - 237
Ph 237a: Gravitational Waves16 January 2001WEEK 2: THE MATHEMATICS UNDERLYING GENERAL RELATIVITY Recommended Reading: 1. Roger D. Blandford and Kip S. Thorne, Applications of Classical Physics [cited henceforth as "Blandford and Thorne"], availab
Caltech - PH - 237
Ph 237b: Gravitational Waves3 April 2002WEEK 11: PHYSICS UNDERLYING INTERFEROMETRIC GW DETECTORS Lectures 19 and 20 by ThorneReading Related to These Lectures:Items in bold are recommended; others are supplementary.1. Proper reference frame
Caltech - PH - 13
Application of Simulation to LIGO Interferometersx xWho am I? Matthew Evans, Ph.D. from Caltech on Lock AcquisitionWhat will I torture you with today? Part 1: Interferometer Simulation The Fabry-Perot Cavity Simulation Ingredients Systems i
Caltech - PH - 237
Application of Simulation to LIGO Interferometersx xWho am I? Matthew Evans, Ph.D. from Caltech on Lock AcquisitionWhat will I torture you with today? Part 1: Interferometer Simulation The Fabry-Perot Cavity Simulation Ingredients Systems i
Caltech - PH - 237
Ph237 - Gravitational Waves Week 1: OverviewKip S. Thorne, Caltech, 7 & 9 January 2001 Via video feed from Cambridge England1Physical Nature of Gravitational Waves - 1 Waves push freely floating objects apart and together Local inertial frame
Caltech - PH - 237
Ph 237b: Gravitational Waves29 May 2002WEEK 19: The Big-Bang Observatory, a Follow-On to LISA; and GW Detection in the ELF Band Using the CMB Polarization Lecture 35 Part 1 by William M. Folkner (JPL) [Big Bang Observatory] Lecture 35 Part 2 by M
Caltech - PH - 237
Ph 237a: Gravitational Waves WEEK 1: OVERVIEW Recommended Reading:9 January 2001Note: Almost all readings will be available for downloading on the web; the url will be given at the end of each reference. 1. Scott A. Hughes, Szabolcs Marka, Peter
Caltech - PH - 237
Ph 237a: Gravitational Waves6 March 2002WEEK 9: SUPERMASSIVE BLACK HOLES PHENOMENOLOGY & GW SOURCES; GWS FROM BIG BANG AMPLIFICATION BY INFLATION Lectures 15 by Phinney, and 16 by ThorneReading Related to Sterls Lecture: Not only are there no
Caltech - PH - 237
Ph 237b: Gravitational Waves8 May 2002WEEK 16: LIGO's Facility Limits; Techniques for LIGO-III Interferometers and Beyond; Resonant-Mass ("Bar") Gravitational-Wave Detectors Lecture 29 Part 1 by Kip [LIGO's Facility Limits] Lecture 29, Part 2 by
Caltech - PH - 237
Ph 237b: Gravitational Waves24 April 2002WEEK 14: LIGO as a Large Science Project; Quantum Optical Noise in Advanced LIGO Interferometers Lecture 25 by Barry Barish [LIGO-II as a Large Science Project]; Lecture 26, by Alessandra Buonanno and Yanb
Caltech - PH - 237
Ph 237b: Gravitational Waves1 May 2002WEEK 15: GW Detection by Doppler Tracking of Spacecraft and Pulsar Timing; LIGO Data Analysis Lecture 27 Part 1 by John Armstrong [GW Detection in LF Band by Doppler Tracking]; Lecture 27, Part 2 by Kip [GW D
Caltech - PH - 237
Ph 237a: Gravitational Waves6 February 2002WEEK 5: THE QUADRUPOLE FORMULA FOR GW GENERATION, PROPAGATION OF GWs THROUGH CURVED SPACETIME AND THE GW STRESS-ENERGY TENSOR Lectures 8 and 9 Recommended Reading: Note: All of this material is on the co
Caltech - PH - 237
Ph 237b: Gravitational Waves8 May 2002WEEK 16: LIGOs Facility Limits; Techniques for LIGO-III Interferometers and Beyond; Resonant-Mass (Bar) Gravitational-Wave Detectors Lecture 29 Part 1 by Kip [LIGOs Facility Limits] Lecture 29, Part 2 by Rona
Caltech - ETD - 05152005
1Chapter 1 IntroductionThe economic outcomes realized by a society are a function of the institutions put in place, the incentives they create, and the behavior of agents in the face of those incentives. In situations where a social planner or gov
Caltech - ETD - 03072006
39Part IIMachine Vision4041Chapter 5Attention for Object Recognition5.1 IntroductionObject recognition with computer algorithms has seen tremendous progress over the past years, both for specic domains such as face recognition (Schneid
Caltech - ETD - 05152005
Institutions, Incentives and Behavior: Essays in Public Economics and Mechanism DesignThesis byPaul J. HealyIn Partial Fulfillment of the Requirements for the Degree of Doctor of PhilosophyCalifornia Institute of Technology Pasadena, Californ
Caltech - ETD - 05262006
121C Analysis of Polyubiquitin Conjugates Reveals that the Rpn10 Substrate Receptor Contributes to the Turnover of Multiple Proteasome TargetsThe publication reprinted here represents the use of MudPIT for a complex mixture of low abundant polypep
Caltech - ETD - 05252006
Unification Of Quantum Information TheoryThesis by Anura AbeyesingheIn Partial Fulfillment of the Requirements for the Degree of Doctor of PhilosophyCalifornia Institute of Technology Pasadena, California 2006 (Defended May 23, 2006)c 2006 An
Caltech - ENG - 061206
Caltech Optical Observatories / NASA Jet Propulsion Laboratory Palomar Adaptive OpticsPalomar Adaptive Optics Test PlanTitleDate Lead Time requested Required conditionsLGS BGS Performance Optimization12/5/2006, V1.0 M. Troy 2 hr On sky with LG