Photon Detection. Array of Photon Detectors. Response Function. Photon Detection. The goal is a simple model for photon detection.

Size: px
Start display at page:

Download "Photon Detection. Array of Photon Detectors. Response Function. Photon Detection. The goal is a simple model for photon detection."

Transcription

1 Photon Detection The goal is a simple model for photon detection. The detector model will have an onset threshold and a saturation level. Photon Detection The photon stream will be treated as a Poisson process. ectures 8 Spring 2002 The ability to detect and measure changes in the photon stream will be analyzed. The performance measures detective quantum efficiency DQE) and noise equivalent power NEP) will be introduced. ecture 8 1 Array of Photon Detectors We will use a simple model with a close-packed array of N detectors, each with area area A, and identical response functions. This simple model will be adequate to demonstrate the basic principles. The expected number of photons at cell k is I k A k T where A k is the area of cell k, I k is the intensity of the photon beam at cell k, and T is the exposure time. Response Function et X be the number of photons that arrive at a detector. et the detector count all photons up to a level. The response function is is Y hx), where { x, x 1 hx), x We will later add an onset threshold to this basic function. ecture 8 2 ecture 8 3

2 The response Y of a detector in the array is a random variable that is measured every T seconds. The number of photons that arrive at a detector element a Poisson random variable X with mean and standard deviation q IAT. The expected value of the response is µ Y E[Y ] P [X k]hk) Insert the model of hk). k e q µ Y + qk e q k k e q µ Y + qk e q k Expand and rearrange. µ Y e q k1 + e q k2 + e q k3 + + e q k There are terms. Term r is of the form e q e q r 1 e q kr r 1 e q 1 ecture 8 4 ecture 8 5 µ Y 1 e q )+ 1 1 e q + Gather terms and rearrange. µ Y e q ) e q ) e q + + ) + The response µ Y as a function of q for a saturation level of 10. Define a function f 1, q) µ Y 1 f 1 q, )e q) ecture 8 6

3 ThresholdT & Saturation evel: S + T 1 0, x < T hx) x T +1, T x<+ T, x + T Calculation of µ Y The equation for the average count now becomes µ Y P [X k]hk) +T 2 µ Y k T +1) qk e q + qk e q kt k+t 1 Modify the function f 1 so that f 1, q) 1 T 1 q k T + T T Response function has the same form: µ Y 1 f 1 q, )e q) ecture 8 8 ecture 8 9 Detector Response µ Y with T 5, 10 Contrast Contrast is determined by the variation in the output when the input changes. The change must be measured at an operating point q 0 : µ Y q 0 + q) µ Y q 0 )+gq 0 ) q and gq 0 ) is the gradient at the operating point. gq 0 ) dµ Y dq e q 0 f 1 df ) 1 qq0 dq qq 0 ecture 8 11

4 f 1, q) 1 T 1 Contrast + T T T Gradient df 1, q) dq 1 T 2 T T +T The derivative of / is 1 /k 1)!. reduced in length by one. Effectively, each term is If we now subtract the derivative from f 1 all that remains is the last term in each sum. f 2, q) f 1 df ) 1 1 dq Solid curve: 10,T 0; dashed curve: 10,T5. These correspond to the response curves in the earlier figures. ecture 8 12 Mean-squared Detector Response E[Y 2 ] h 2 k)p [X k] k 2qk e q + 2qk e q k This can be expressed in terms of a function f 3, q) as E[Y 2 ] 2 1 f 3 e q) where f 3, q) 1 1 q 1+3 k ) 1 n 2 2n +1) n0 ecture 8 15

5 Variance of the Detector Response σ 2 Y E[Y 2 ] µ 2 Y Comparative Noise evel The action of the detector and internally produced noise contribute to the variance of the detector output. 2 [ 1 f 3 e q ) 1 f 1 e q ) 2] The upper figure shows E[Y 2 ] solid) and µ 2 Y dashed) for a quantum detector with 10 and T 0. The lower curve shows the variance, which is the difference between the two curves in the upper figure. The detector noise performance can be described by the comparative noise level. ε g2 σx 2 σy 2 + σ2 n ecture 8 16 ecture 8 17 Comparative Noise evel The variance of the input is σx 2 q. The gain is the response gradient gq) e q f 2, q) The variance of the output in the absence of internal noise is σy 2 [ 2 1 f 3 e q ) 1 f 1 e q ) 2] The comparative noise level is ε g2 σ 2 X σ 2 Y + σ2 n q e q f 2, q) ) 2 2 [ 1 f 3 e q ) 1 f 1 e q ) 2] + σ 2 n The second law of thermodynamics requires that the output noise be at least as large as the noise that is actually present at the input, so that the comparative noise level is always less than unity. ecture 8 18

Detector. Detector Model. Estimator. Detective Quantum Efficiency. An input photon stream X is presented to the detector.

Detector. Detector Model. Estimator. Detective Quantum Efficiency. An input photon stream X is presented to the detector. Detector An input photon stream X is presented to the detector. Detective Quantum Efficiency Lecture 9 Spring 2002 X is a random variable with a Poisson distribution. P (X k) qk k! e q where q λ The response

More information

Detective Quantum Efficiency

Detective Quantum Efficiency Detective Quantum Efficiency Lecture 9 Spring 2002 Detector An input photon stream X is presented to the detector. X is a random variable with a Poisson distribution. P (X = k) = qk k! e q where q = λaτ

More information

Chapter 4. Repeated Trials. 4.1 Introduction. 4.2 Bernoulli Trials

Chapter 4. Repeated Trials. 4.1 Introduction. 4.2 Bernoulli Trials Chapter 4 Repeated Trials 4.1 Introduction Repeated indepentent trials in which there can be only two outcomes are called Bernoulli trials in honor of James Bernoulli (1654-1705). As we shall see, Bernoulli

More information

Effects of Transfer Gate Spill Back in Low Light High Performances CMOS Image Sensors

Effects of Transfer Gate Spill Back in Low Light High Performances CMOS Image Sensors Effects of Transfer Gate Spill Back in Low Light High Performances CMOS Image Sensors Photon Counting, Low Flux and High Dynamic Range Optoelectronic Detectors Workshop Toulouse 17th November 2016 Julien

More information

Counting Statistics and Error Prediction

Counting Statistics and Error Prediction Counting Statistics and Error Prediction Outline Characterization of data Statistical models Error propagation Optimization of counting experiments Energy resolution Detection efficiency Dead time Characterization

More information

Variance. Standard deviation VAR = = value. Unbiased SD = SD = 10/23/2011. Functional Connectivity Correlation and Regression.

Variance. Standard deviation VAR = = value. Unbiased SD = SD = 10/23/2011. Functional Connectivity Correlation and Regression. 10/3/011 Functional Connectivity Correlation and Regression Variance VAR = Standard deviation Standard deviation SD = Unbiased SD = 1 10/3/011 Standard error Confidence interval SE = CI = = t value for

More information

Lecture 9. PMTs and Laser Noise. Lecture 9. Photon Counting. Photomultiplier Tubes (PMTs) Laser Phase Noise. Relative Intensity

Lecture 9. PMTs and Laser Noise. Lecture 9. Photon Counting. Photomultiplier Tubes (PMTs) Laser Phase Noise. Relative Intensity s and Laser Phase Phase Density ECE 185 Lasers and Modulators Lab - Spring 2018 1 Detectors Continuous Output Internal Photoelectron Flux Thermal Filtered External Current w(t) Sensor i(t) External System

More information

Photon noise in holography. By Daniel Marks, Oct

Photon noise in holography. By Daniel Marks, Oct Photon noise in holography By Daniel Marks, Oct 8 009 The Poisson popcorn Process Photons arriving at a detector have similar statistics to popcorn popping. At each time instant, there is an independent

More information

AanumntBAasciAs. l e t e s auas trasuarbe, amtima*. pay Bna. aaeh t!iacttign. Xat as eling te Trndi'aBd^glit!

AanumntBAasciAs. l e t e s auas trasuarbe, amtima*. pay Bna. aaeh t!iacttign. Xat as eling te Trndi'aBd^glit! - [ - --- --- ~ - 5 4 G 4? G 8 0 0 0 7 0 - Q - - - 6 8 7 2 75 00 - [ 7-6 - - Q - ] z - 9 - G - 0 - - z / - ] G / - - 4-6 7 - z - 6 - - z - - - - - - G z / - - - G 0 Zz 4 z4 5? - - Z z 2 - - {- 9 9? Z G

More information

Error propagation. Alexander Khanov. October 4, PHYS6260: Experimental Methods is HEP Oklahoma State University

Error propagation. Alexander Khanov. October 4, PHYS6260: Experimental Methods is HEP Oklahoma State University Error propagation Alexander Khanov PHYS660: Experimental Methods is HEP Oklahoma State University October 4, 017 Why error propagation? In many cases we measure one thing and want to know something else

More information

Pulse characterization with Wavelet transforms combined with classification using binary arrays

Pulse characterization with Wavelet transforms combined with classification using binary arrays Pulse characterization with Wavelet transforms combined with classification using binary arrays Overview Wavelet Transformation Creating binary arrays out of and how to deal with them An estimator for

More information

estec NIRSpec Technical Note NTN Spectral intensity of the MSA glow sources Abstract:

estec NIRSpec Technical Note NTN Spectral intensity of the MSA glow sources Abstract: NIRSpec Technical Note NTN-2013-014 Authors: P. Ferruit & G. Giardino Date of Issue: 29.11.2013 Version: 1 estec European Space Research and Technology Centre Keplerlaan 1 2201 AZ Noordwijk The Netherlands

More information

Astronomical Observing Techniques 2017 Lecture 9: Silicon Eyes 1

Astronomical Observing Techniques 2017 Lecture 9: Silicon Eyes 1 Astronomical Observing Techniques 2017 Lecture 9: Silicon Eyes 1 Christoph U. Keller keller@strw.leidenuniv.nl Content 1. Detector Types 2. Crystal La>ces 3. Electronic Bands 4. Fermi Energy and Fermi

More information

Counting Photons to Calibrate a Photometer for Stellar Intensity Interferometry

Counting Photons to Calibrate a Photometer for Stellar Intensity Interferometry Counting Photons to Calibrate a Photometer for Stellar Intensity Interferometry A Senior Project Presented to the Department of Physics California Polytechnic State University, San Luis Obispo In Partial

More information

OPTICS AND Optical Instrumentation

OPTICS AND Optical Instrumentation OPTICS AND Optical Instrumentation Optical imaging is the manipulation of light to elucidate the structures of objects History of Optics Optical Instrumentation light sources Optical Instrumentation detectors

More information

Phys 4061 Lecture Thirteen Photodetectors

Phys 4061 Lecture Thirteen Photodetectors Phys 4061 Lecture Thirteen Photodetectors Recall properties of indirect band gap materials that are used as photodetectors Photoelectric Effect in Semiconductors hν > Eg + χ χ is the electron affinity

More information

Part 1: Logic and Probability

Part 1: Logic and Probability Part 1: Logic and Probability In some sense, probability subsumes logic: While a probability can be seen as a measure of degree of truth a real number between 0 and 1 logic deals merely with the two extreme

More information

1 Photon optics! Photons and modes Photon properties Photon streams and statistics

1 Photon optics! Photons and modes Photon properties Photon streams and statistics 1 Photons and modes Photon properties Photon optics! Photon streams and statistics 2 Photon optics! Photons and modes Photon properties Energy, polarization, position, momentum, interference, time Photon

More information

Lecture 23. CMOS Logic Gates and Digital VLSI I

Lecture 23. CMOS Logic Gates and Digital VLSI I ecture 3 CMOS ogic Gates and Digital SI I In this lecture you will learn: Digital ogic The CMOS Inverter Charge and Discharge Dynamics Power Dissipation Digital evels and Noise NFET Inverter Cut-off Saturation

More information

Generalized Linear Models (1/29/13)

Generalized Linear Models (1/29/13) STA613/CBB540: Statistical methods in computational biology Generalized Linear Models (1/29/13) Lecturer: Barbara Engelhardt Scribe: Yangxiaolu Cao When processing discrete data, two commonly used probability

More information

AST1100 Lecture Notes

AST1100 Lecture Notes AST11 Lecture Notes Part 1G Quantum gases Questions to ponder before the lecture 1. If hydrostatic equilibrium in a star is lost and gravitational forces are stronger than pressure, what will happen with

More information

UC Berkeley Department of Electrical Engineering and Computer Science. EE 126: Probablity and Random Processes. Solutions 9 Spring 2006

UC Berkeley Department of Electrical Engineering and Computer Science. EE 126: Probablity and Random Processes. Solutions 9 Spring 2006 UC Berkeley Department of Electrical Engineering and Computer Science EE 6: Probablity and Random Processes Solutions 9 Spring 006 Exam format The second midterm will be held in class on Thursday, April

More information

Slide Set Data Converters. Digital Enhancement Techniques

Slide Set Data Converters. Digital Enhancement Techniques 0 Slide Set Data Converters Digital Enhancement Techniques Introduction Summary Error Measurement Trimming of Elements Foreground Calibration Background Calibration Dynamic Matching Decimation and Interpolation

More information

Statistics of Accumulating Signal

Statistics of Accumulating Signal Instrument Science Report NICMOS 98-008 Statistics of Accumulating Signal W.B. Sparks, STScI May 1998 ABSTRACT NICMOS detectors accumulate charge which can be non-destructively. The charge accumulation

More information

Chapter 2: Statistical Methods. 4. Total Measurement System and Errors. 2. Characterizing statistical distribution. 3. Interpretation of Results

Chapter 2: Statistical Methods. 4. Total Measurement System and Errors. 2. Characterizing statistical distribution. 3. Interpretation of Results 36 Chapter : Statistical Methods 1. Introduction. Characterizing statistical distribution 3. Interpretation of Results 4. Total Measurement System and Errors 5. Regression Analysis 37 1.Introduction The

More information

noise = function whose amplitude is is derived from a random or a stochastic process (i.e., not deterministic)

noise = function whose amplitude is is derived from a random or a stochastic process (i.e., not deterministic) SIMG-716 Linear Imaging Mathematics I, Handout 05 1 1-D STOCHASTIC FUCTIOS OISE noise = function whose amplitude is is derived from a random or a stochastic process (i.e., not deterministic) Deterministic:

More information

Solutions for Exercise session I

Solutions for Exercise session I Solutions for Exercise session I 1. The maximally polarisation-entangled photon state can be written as Ψ = 1 ( H 1 V V 1 H ). Show that the state is invariant (i.e. still maximally entangled) after a

More information

ΔP(x) Δx. f "Discrete Variable x" (x) dp(x) dx. (x) f "Continuous Variable x" Module 3 Statistics. I. Basic Statistics. A. Statistics and Physics

ΔP(x) Δx. f Discrete Variable x (x) dp(x) dx. (x) f Continuous Variable x Module 3 Statistics. I. Basic Statistics. A. Statistics and Physics Module 3 Statistics I. Basic Statistics A. Statistics and Physics 1. Why Statistics Up to this point, your courses in physics and engineering have considered systems from a macroscopic point of view. For

More information

Path Entanglement. Liat Dovrat. Quantum Optics Seminar

Path Entanglement. Liat Dovrat. Quantum Optics Seminar Path Entanglement Liat Dovrat Quantum Optics Seminar March 2008 Lecture Outline Path entangled states. Generation of path entangled states. Characteristics of the entangled state: Super Resolution Beating

More information

CSE 312, Winter 2011, W.L.Ruzzo. 8. Average-Case Analysis of Algorithms + Randomized Algorithms

CSE 312, Winter 2011, W.L.Ruzzo. 8. Average-Case Analysis of Algorithms + Randomized Algorithms CSE 312, Winter 2011, W.L.Ruzzo 8. Average-Case Analysis of Algorithms + Randomized Algorithms 1 insertion sort Array A[1]..A[n] for i = 1..n-1 { T = A[i] Sorted j swap j = i-1 compare while j >= 0 &&

More information

Dynamics of star clusters containing stellar mass black holes: 1. Introduction to Gravitational Waves

Dynamics of star clusters containing stellar mass black holes: 1. Introduction to Gravitational Waves Dynamics of star clusters containing stellar mass black holes: 1. Introduction to Gravitational Waves July 25, 2017 Bonn Seoul National University Outline What are the gravitational waves? Generation of

More information

Observation of flavor swap process in supernova II neutrino spectra

Observation of flavor swap process in supernova II neutrino spectra Observation of flavor swap process in supernova II neutrino spectra David B. Cline and George Fuller Abstract. We review the concept of quantum flavor swap in a SNII explosion. There will be a specific

More information

Particles and Deep Inelastic Scattering

Particles and Deep Inelastic Scattering Particles and Deep Inelastic Scattering University HUGS - JLab - June 2010 June 2010 HUGS 1 Sum rules You can integrate the structure functions and recover quantities like the net number of quarks. Momentum

More information

Photon Instrumentation. First Mexican Particle Accelerator School Guanajuato Oct 6, 2011

Photon Instrumentation. First Mexican Particle Accelerator School Guanajuato Oct 6, 2011 Photon Instrumentation First Mexican Particle Accelerator School Guanajuato Oct 6, 2011 Outline The Electromagnetic Spectrum Photon Detection Interaction of Photons with Matter Photoelectric Effect Compton

More information

Astrophysics I ASTR:3771 Fall 2014

Astrophysics I ASTR:3771 Fall 2014 Astrophysics I ASTR:3771 Fall 2014 Prof. Kaaret 702 Van Allen Hall 335-1985 philip-kaaret@uiowa.edu Office hours: Tuesday 1:30-2:30 pm, Wednesday 9-11 am, or by appointment, or drop by. Topics We will

More information

CSE 421, Spring 2017, W.L.Ruzzo. 8. Average-Case Analysis of Algorithms + Randomized Algorithms

CSE 421, Spring 2017, W.L.Ruzzo. 8. Average-Case Analysis of Algorithms + Randomized Algorithms CSE 421, Spring 2017, W.L.Ruzzo 8. Average-Case Analysis of Algorithms + Randomized Algorithms 1 outline and goals 1) Probability tools you've seen allow formal definition of "average case" running time

More information

ECON 3150/4150, Spring term Lecture 6

ECON 3150/4150, Spring term Lecture 6 ECON 3150/4150, Spring term 2013. Lecture 6 Review of theoretical statistics for econometric modelling (II) Ragnar Nymoen University of Oslo 31 January 2013 1 / 25 References to Lecture 3 and 6 Lecture

More information

Basic concepts of probability theory

Basic concepts of probability theory Basic concepts of probability theory Random variable discrete/continuous random variable Transform Z transform, Laplace transform Distribution Geometric, mixed-geometric, Binomial, Poisson, exponential,

More information

Final Solutions Fri, June 8

Final Solutions Fri, June 8 EE178: Probabilistic Systems Analysis, Spring 2018 Final Solutions Fri, June 8 1. Small problems (62 points) (a) (8 points) Let X 1, X 2,..., X n be independent random variables uniformly distributed on

More information

18.440: Lecture 26 Conditional expectation

18.440: Lecture 26 Conditional expectation 18.440: Lecture 26 Conditional expectation Scott Sheffield MIT 1 Outline Conditional probability distributions Conditional expectation Interpretation and examples 2 Outline Conditional probability distributions

More information

Regression Analysis: Basic Concepts

Regression Analysis: Basic Concepts The simple linear model Regression Analysis: Basic Concepts Allin Cottrell Represents the dependent variable, y i, as a linear function of one independent variable, x i, subject to a random disturbance

More information

Introduction Growthequations Decay equations Forming differential equations Case studies Shifted equations Test INU0115/515 (MATHS 2)

Introduction Growthequations Decay equations Forming differential equations Case studies Shifted equations Test INU0115/515 (MATHS 2) GROWTH AND DECAY CALCULUS 12 INU0115/515 (MATHS 2) Dr Adrian Jannetta MIMA CMath FRAS Growth and Decay 1/ 24 Adrian Jannetta Introduction Some of the simplest systems that can be modelled by differential

More information

5 Error Propagation We start from eq , which shows the explicit dependence of g on the measured variables t and h. Thus.

5 Error Propagation We start from eq , which shows the explicit dependence of g on the measured variables t and h. Thus. 5 Error Propagation We start from eq..4., which shows the explicit dependence of g on the measured variables t and h. Thus g(t,h) = h/t eq..5. The simplest way to get the error in g from the error in t

More information

EXPOSURE TIME ESTIMATION

EXPOSURE TIME ESTIMATION ASTR 511/O Connell Lec 12 1 EXPOSURE TIME ESTIMATION An essential part of planning any observation is to estimate the total exposure time needed to satisfy your scientific goal. General considerations

More information

Statistical Techniques II EXST7015 Simple Linear Regression

Statistical Techniques II EXST7015 Simple Linear Regression Statistical Techniques II EXST7015 Simple Linear Regression 03a_SLR 1 Y - the dependent variable 35 30 25 The objective Given points plotted on two coordinates, Y and X, find the best line to fit the data.

More information

The kinetic equation (Lecture 11)

The kinetic equation (Lecture 11) The kinetic equation (Lecture 11) January 29, 2016 190/441 Lecture outline In the preceding lectures we focused our attention on a single particle motion. In this lecture, we will introduce formalism for

More information

External (differential) quantum efficiency Number of additional photons emitted / number of additional electrons injected

External (differential) quantum efficiency Number of additional photons emitted / number of additional electrons injected Semiconductor Lasers Comparison with LEDs The light emitted by a laser is generally more directional, more intense and has a narrower frequency distribution than light from an LED. The external efficiency

More information

arxiv:gr-qc/ v1 16 Feb 2007

arxiv:gr-qc/ v1 16 Feb 2007 International Journal of Modern Physics D c World Scientific Publishing Company arxiv:gr-qc/0702096v1 16 Feb 2007 Data Analysis of Gravitational Waves Using A Network of Detectors Linqing Wen Max Planck

More information

Optical interference and nonlinearities in quantum-well infrared photodetectors

Optical interference and nonlinearities in quantum-well infrared photodetectors Physica E 7 (2000) 115 119 www.elsevier.nl/locate/physe Optical interference and nonlinearities in quantum-well infrared photodetectors M. Ershov a;, H.C. Liu b, A.G.U. Perera a, S.G. Matsik a a Department

More information

Wave Packet with a Resonance

Wave Packet with a Resonance Wave Packet with a Resonance I just wanted to tell you how one can study the time evolution of the wave packet around the resonance region quite convincingly. This in my mind is the most difficult problem

More information

Nuclear Instruments and Methods in Physics Research A 417 (1998) 86 94

Nuclear Instruments and Methods in Physics Research A 417 (1998) 86 94 Nuclear Instruments and Methods in Physics Research A 417 (1998) 86 94 Experimental determination of detector gain, zero frequency detective quantum efficiency, and spectral compatibility of phosphor screens:

More information

Exponential Smoothing. INSR 260, Spring 2009 Bob Stine

Exponential Smoothing. INSR 260, Spring 2009 Bob Stine Exponential Smoothing INSR 260, Spring 2009 Bob Stine 1 Overview Smoothing Exponential smoothing Model behind exponential smoothing Forecasts and estimates Hidden state model Diagnostic: residual plots

More information

Thermal noise and correlations in photon detection

Thermal noise and correlations in photon detection Thermal noise and correlations in photon detection Jonas Zmuidzinas The standard expressions for the noise that is due to photon fluctuations in thermal background radiation typically apply only for a

More information

Metal Artifact Reduction and Dose Efficiency Improvement on Photon Counting Detector CT using an Additional Tin Filter

Metal Artifact Reduction and Dose Efficiency Improvement on Photon Counting Detector CT using an Additional Tin Filter Metal Artifact Reduction and Dose Efficiency Improvement on Photon Counting Detector CT using an Additional Tin Filter Wei Zhou, Dilbar Abdurakhimova, Kishore Rajendran, Cynthia McCollough, Shuai Leng

More information

Lecture 8. The Second Law of Thermodynamics; Energy Exchange

Lecture 8. The Second Law of Thermodynamics; Energy Exchange Lecture 8 The Second Law of Thermodynamics; Energy Exchange The second law of thermodynamics Statistics of energy exchange General definition of temperature Why heat flows from hot to cold Reading for

More information

Increasing your confidence Proving that data is single molecule. Chem 184 Lecture David Altman 5/27/08

Increasing your confidence Proving that data is single molecule. Chem 184 Lecture David Altman 5/27/08 Increasing your confidence Proving that data is single molecule Chem 184 Lecture David Altman 5/27/08 Brief discussion/review of single molecule fluorescence Statistical analysis of your fluorescence data

More information

A Fast Algorithm for Cosmic Rays Removal from Single Images

A Fast Algorithm for Cosmic Rays Removal from Single Images A Fast Algorithm for Cosmic Rays Removal from Single Images Wojtek Pych David Dunlap Observatory, University of Toronto P.O. Box 360, Richmond Hill, Ontario, Canada L4C 4Y6 and Copernicus Astronomical

More information

Infrared thermography

Infrared thermography Infrared thermography In microwave radiometry hν

More information

Thermodynamic Energy Equation

Thermodynamic Energy Equation Thermodynamic Energy Equation The temperature tendency is = u T x v T y w T z + dt dt (1) where dt/dt is the individual derivative of temperature. This temperature change experienced by the air parcel

More information

Charm and Beauty Structure of the proton

Charm and Beauty Structure of the proton International Conference Heavy Quarks and Leptons München, 16-20 October 2006 Riccardo Brugnera Padova University and INFN on behalf of the H1 and ZEUS Collaborations Charm and Beauty Structure of the

More information

Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015)

Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015) Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015) Interaction of x-ray with matter: - Photoelectric absorption - Elastic (coherent) scattering (Thomson Scattering) - Inelastic (incoherent) scattering

More information

12 Count-Min Sketch and Apriori Algorithm (and Bloom Filters)

12 Count-Min Sketch and Apriori Algorithm (and Bloom Filters) 12 Count-Min Sketch and Apriori Algorithm (and Bloom Filters) Many streaming algorithms use random hashing functions to compress data. They basically randomly map some data items on top of each other.

More information

1 The purpose and circumstances of the experiment

1 The purpose and circumstances of the experiment Experiments with MSS. Tokovinin, V. Kornilov Version. Oct., 4 (experiments.tex) The purpose and circumstances of the experiment s more experience is gained with operating MSS turbulence profiler, the method

More information

Proposal of Michelson-Morley experiment via single photon. interferometer: Interpretation of Michelson-Morley

Proposal of Michelson-Morley experiment via single photon. interferometer: Interpretation of Michelson-Morley Proposal of Michelson-Morley experiment via single photon interferometer: Interpretation of Michelson-Morley experimental results using de Broglie-Bohm picture Masanori Sato Honda Electronics Co., Ltd.,

More information

arxiv:astro-ph/ v1 12 Nov 2003

arxiv:astro-ph/ v1 12 Nov 2003 A Fast Algorithm for Cosmic Rays Removal from Single Images Wojtek Pych arxiv:astro-ph/0311290v1 12 Nov 2003 David Dunlap Observatory, University of Toronto P.O. Box 360, Richmond Hill, Ontario, Canada

More information

Probability theory. References:

Probability theory. References: Reasoning Under Uncertainty References: Probability theory Mathematical methods in artificial intelligence, Bender, Chapter 7. Expert systems: Principles and programming, g, Giarratano and Riley, pag.

More information

Parametric down-conversion

Parametric down-conversion Parametric down-conversion 1 Introduction You have seen that laser light, for all its intensity and coherence, gave us the same PP(mm) counts distribution as a thermal light source with a high fluctuation

More information

EE 637 Final April 30, Spring Each problem is worth 20 points for a total score of 100 points

EE 637 Final April 30, Spring Each problem is worth 20 points for a total score of 100 points EE 637 Final April 30, Spring 2018 Name: Instructions: This is a 120 minute exam containing five problems. Each problem is worth 20 points for a total score of 100 points You may only use your brain and

More information

Detection of X-Rays. Solid state detectors Proportional counters Microcalorimeters Detector characteristics

Detection of X-Rays. Solid state detectors Proportional counters Microcalorimeters Detector characteristics Detection of X-Rays Solid state detectors Proportional counters Microcalorimeters Detector characteristics Solid State X-ray Detectors X-ray interacts in material to produce photoelectrons which are collected

More information

[Chapter 6. Functions of Random Variables]

[Chapter 6. Functions of Random Variables] [Chapter 6. Functions of Random Variables] 6.1 Introduction 6.2 Finding the probability distribution of a function of random variables 6.3 The method of distribution functions 6.5 The method of Moment-generating

More information

Supplementary Figure 1. Characterization of the single-photon quantum light source based on spontaneous parametric down-conversion (SPDC).

Supplementary Figure 1. Characterization of the single-photon quantum light source based on spontaneous parametric down-conversion (SPDC). .2 Classical light source.8 g (2) ().6.4.2 EMCCD SPAD 2 3.2.4.6.8..2.4.6.8.2 Mean number of photon pairs per pump pulse 4 5 6 7 8 9 2 3 4 Supplementary Figure. Characterization of the single-photon quantum

More information

Partial Differentiation

Partial Differentiation CHAPTER 7 Partial Differentiation From the previous two chapters we know how to differentiate functions of one variable But many functions in economics depend on several variables: output depends on both

More information

Astronomy 203 practice final examination

Astronomy 203 practice final examination Astronomy 203 practice final examination Fall 1999 If this were a real, in-class examination, you would be reminded here of the exam rules, which are as follows: You may consult only one page of formulas

More information

Lecture 1: Introduction to Sublinear Algorithms

Lecture 1: Introduction to Sublinear Algorithms CSE 522: Sublinear (and Streaming) Algorithms Spring 2014 Lecture 1: Introduction to Sublinear Algorithms March 31, 2014 Lecturer: Paul Beame Scribe: Paul Beame Too much data, too little time, space for

More information

The Euler Equation. Using the additive property of the internal energy U, we can derive a useful thermodynamic relation the Euler equation.

The Euler Equation. Using the additive property of the internal energy U, we can derive a useful thermodynamic relation the Euler equation. The Euler Equation Using the additive property of the internal energy U, we can derive a useful thermodynamic relation the Euler equation. Let us differentiate this extensivity condition with respect to

More information

Computer Intensive Methods in Mathematical Statistics

Computer Intensive Methods in Mathematical Statistics Computer Intensive Methods in Mathematical Statistics Department of mathematics johawes@kth.se Lecture 16 Advanced topics in computational statistics 18 May 2017 Computer Intensive Methods (1) Plan of

More information

AQA Physics /7408

AQA Physics /7408 AQA Physics - 7407/7408 Module 10: Medical physics You should be able to demonstrate and show your understanding of: 10.1 Physics of the eye 10.1.1 Physics of vision The eye as an optical refracting system,

More information

nm are produced. When the condition for degenerate

nm are produced. When the condition for degenerate VOLUME 61, NUMBER 1 PHYSCAL REVEW LETTERS 4 JULY 1988 Violation of Bells nequality and Classical Probability in a Two-Photon Correlation Experiment Z. Y. Ou and L. Mandel Department of Physics and Astronomy,

More information

1 1D Schrödinger equation: Particle in an infinite box

1 1D Schrödinger equation: Particle in an infinite box 1 OF 5 1 1D Schrödinger equation: Particle in an infinite box Consider a particle of mass m confined to an infinite one-dimensional well of width L. The potential is given by V (x) = V 0 x L/2, V (x) =

More information

Portable Instrument for Online Investigations of Optical Properties of Airborne Particles

Portable Instrument for Online Investigations of Optical Properties of Airborne Particles Portable Instrument for Online Investigations of Optical Properties of Airborne Particles Julian Robertz*, Aleksandar Duric, Martin Allemann Siemens Schweiz AG, Building Technologies Division, Zug, Switzerland

More information

UC Berkeley Department of Electrical Engineering and Computer Science. EE 126: Probablity and Random Processes. Problem Set 8 Fall 2007

UC Berkeley Department of Electrical Engineering and Computer Science. EE 126: Probablity and Random Processes. Problem Set 8 Fall 2007 UC Berkeley Department of Electrical Engineering and Computer Science EE 6: Probablity and Random Processes Problem Set 8 Fall 007 Issued: Thursday, October 5, 007 Due: Friday, November, 007 Reading: Bertsekas

More information

Simple Linear Regression. Material from Devore s book (Ed 8), and Cengagebrain.com

Simple Linear Regression. Material from Devore s book (Ed 8), and Cengagebrain.com 12 Simple Linear Regression Material from Devore s book (Ed 8), and Cengagebrain.com The Simple Linear Regression Model The simplest deterministic mathematical relationship between two variables x and

More information

Detecting high energy photons. Interactions of photons with matter Properties of detectors (with examples)

Detecting high energy photons. Interactions of photons with matter Properties of detectors (with examples) Detecting high energy photons Interactions of photons with matter Properties of detectors (with examples) Interactions of high energy photons with matter Cross section/attenution length/optical depth Photoelectric

More information

LOW ENERGY SOLAR NEUTRINOS WITH BOREXINO. Lea Di Noto on behalf of the Borexino collaboration

LOW ENERGY SOLAR NEUTRINOS WITH BOREXINO. Lea Di Noto on behalf of the Borexino collaboration LOW ENERGY SOLAR NEUTRINOS WITH BOREXINO Lea Di Noto on behalf of the Borexino collaboration Vulcano Workshop 20 th -26 th May 2018 [cm -2 s -1 MeV -1 ] SOLAR NEUTRINOS Electrons neutrinos are produced

More information

σx=2.5cm, slpx =33mrd

σx=2.5cm, slpx =33mrd NOTE 0221 MUON COOLING EXPERIMENT- MC SIMULATION of BEAM PARTICLE ID L. Cremaldi *, D.Summers University of Mississippi Oct 10, 2001 I. INTRODUCTION In future tests of a muon cooling channel e,. beam tagging

More information

Chi-square is defined as the sum of the square of the (observed values - expected values) divided by the expected values, or

Chi-square is defined as the sum of the square of the (observed values - expected values) divided by the expected values, or 2016 Midterm Exam (100 points total) Name: Astronomy/Planetary Sciences 518/418 Profs. Hinz/Rieke If you need more space, use the reverse side of the relevant page, but let us know by writing (over) at

More information

Lecture 2. Frequency problems

Lecture 2. Frequency problems 1 / 43 Lecture 2. Frequency problems Ricard Gavaldà MIRI Seminar on Data Streams, Spring 2015 Contents 2 / 43 1 Frequency problems in data streams 2 Approximating inner product 3 Computing frequency moments

More information

Uncertainty in Measurements

Uncertainty in Measurements Uncertainty in Measurements Joshua Russell January 4, 010 1 Introduction Error analysis is an important part of laboratory work and research in general. We will be using probability density functions PDF)

More information

Basics of Infrared Detection

Basics of Infrared Detection 2 Basics of Infrared Detection Before the in-depth analyses of quantum well, ISBT, and QWIP a specific infrared detector we first discuss the general concept of how the temperature of an object influences

More information

POL 213: Research Methods

POL 213: Research Methods Brad 1 1 Department of Political Science University of California, Davis April 15, 2008 Some Matrix Basics What is a matrix? A rectangular array of elements arranged in rows and columns. 55 900 0 67 1112

More information

Inference Tutorial 2

Inference Tutorial 2 Inference Tutorial 2 This sheet covers the basics of linear modelling in R, as well as bootstrapping, and the frequentist notion of a confidence interval. When working in R, always create a file containing

More information

Optimal combination forecasts for hierarchical time series

Optimal combination forecasts for hierarchical time series Optimal combination forecasts for hierarchical time series Rob J. Hyndman Roman A. Ahmed Department of Econometrics and Business Statistics Outline 1 Review of hierarchical forecasting 2 3 Simulation study

More information

A Fast Algorithm for Cosmic-Ray Removal from Single Images

A Fast Algorithm for Cosmic-Ray Removal from Single Images Publications of the Astronomical Society of the Pacific, 116:148 153, 2004 February 2004. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. A Fast Algorithm for Cosmic-Ray

More information

Introduction to Computational Finance and Financial Econometrics Matrix Algebra Review

Introduction to Computational Finance and Financial Econometrics Matrix Algebra Review You can t see this text! Introduction to Computational Finance and Financial Econometrics Matrix Algebra Review Eric Zivot Spring 2015 Eric Zivot (Copyright 2015) Matrix Algebra Review 1 / 54 Outline 1

More information

Statistics, Data Analysis, and Simulation SS 2013

Statistics, Data Analysis, and Simulation SS 2013 Statistics, Data Analysis, and Simulation SS 2013 08.128.730 Statistik, Datenanalyse und Simulation Dr. Michael O. Distler Mainz, May 21, 2013 3. Parameter estimation 1 Consistency:

More information

Random Variables. P(x) = P[X(e)] = P(e). (1)

Random Variables. P(x) = P[X(e)] = P(e). (1) Random Variables Random variable (discrete or continuous) is used to derive the output statistical properties of a system whose input is a random variable or random in nature. Definition Consider an experiment

More information

This is a Gaussian probability centered around m = 0 (the most probable and mean position is the origin) and the mean square displacement m 2 = n,or

This is a Gaussian probability centered around m = 0 (the most probable and mean position is the origin) and the mean square displacement m 2 = n,or Physics 7b: Statistical Mechanics Brownian Motion Brownian motion is the motion of a particle due to the buffeting by the molecules in a gas or liquid. The particle must be small enough that the effects

More information

ECE302 Spring 2015 HW10 Solutions May 3,

ECE302 Spring 2015 HW10 Solutions May 3, ECE32 Spring 25 HW Solutions May 3, 25 Solutions to HW Note: Most of these solutions were generated by R. D. Yates and D. J. Goodman, the authors of our textbook. I have added comments in italics where

More information

Tomography and Reconstruction

Tomography and Reconstruction Tomography and Reconstruction Lecture Overview Applications Background/history of tomography Radon Transform Fourier Slice Theorem Filtered Back Projection Algebraic techniques Measurement of Projection

More information

Measuring Colocalization within Fluorescence Microscopy Images

Measuring Colocalization within Fluorescence Microscopy Images from photonics.com: 03/01/2007 http://www.photonics.com/article.aspx?aid=39341 Measuring Colocalization within Fluorescence Microscopy Images Two-color fluorescence-based methods are uncovering molecular

More information