The Analysis of Quasar Absorption Line Spectra
Chris ChurchillAssistant Professor of Astronomy
A TEXT BOOK ON RESEARCH INTO THE INTERGALACTIC AND INTERSTELLAR GASEOUS BARYONIC COMPONENTS OF THE UNIVERSE FOR GRADUATE STUDENTS AND ADVANCED UNDERGRADS
The book is scheduled to be delivered to Cambridge University Press in the January - April of 2008 (I had an accident and broke my hand- delaying the book even further - again) and will be part of its Cambridge Astrophysic Series.
All material Copywrite (C) Christopher W. Churchill (2008).
Preliminary Message to the Reader
Due the lack of an up-to-date reference book on the research methods employing the methods of quasar absorption lines, I have undertaken the task of writing one. The notes are derived from my lectures and research experience, and are targeted toward researchers of astronomy and astrophsyics. The book includesSince the last iteration, the book has changed significantly, so I have taken the chapters off line.The physics of radiative transfer, atomic systems (sorry, no molecules), and gas structures with focus on application for spectral analysis.
Physically motivated distribution functions. Analysis methods such as chi-square least squares fitting and maximum likelihood analysis. The observable features in quasar spectra, the ionization breaks, GP trough, Lyman leaks, absorption line curve of growth.
Fundamentals of spectroscopic theory, spectrograph design, characteristic of spectra, reduction of spectra, and spectroscopic analysis of absorption and emission features
introduce the cosmological setting and experimental methods of quasar absorption lines, with emphasis on analysis to extract quantities based upon the physics of radiative transfer, atomic absorption properties, and cosmological evolution.
If you are interested in obtaining any of the material, please contact me via email. Let me know which chapter or sections you would like. I provide an outline below.
I am interested in proof readers! If you wish to contribute, please email me. I will of course give all contributers their very due acknowledgments.
Contents
Subsections are not listed...Chaper 1: Introduction
1.1 Quasars and Astronomy(10% complete)
1.2 Qualitative History of the Gaseous Universe
1.3 The Tool of Quasar Absorption Lines
1.4 Taxonomy of Absorbers
Chaper 2: The Cosmography
2.1 The Metric(100% complete)
2.2 Relativistic Dynamics
2.3 Parameterized Cosmology
2.4 H_0 and the Three Omega's
2.5 Scale Factor and Redshift
2.6 Dynamics and Redshift
2.7 Time and Redshift
2.8 Distance and Redshift
2.9 Velocity and Redshift
2.10 Volume and Redshift
2.11 Probability of Line of Sight Intersection
2.12 Luminosity and Surface Brightness
Chaper 3: Data and Parameter Estimation
3.1 Statistical Descriptors of Data(100% complete)
3.2 Common Distribution Functions
3.3 Confidence Intervals and Levels
3.4 Statistical Tests
3.5 The Sensitivity Function
3.6 Parameterized Distribution Functions
3.7 Maximum Likelihood Method
3.8 Chi-Square Minimization
Chaper 4: Chemical Elements and Atomic Structure
4.1 Abundances(50% complete; additional sections may be added)
4.2 Hydrogen and Hydrogen-Like Ions
4.3 Wave Model of the Atom
4.4 Grotrian Diagrams
Appendix: Ionization Potentials
Chaper 5: Radiative Transfer
5.1 Defining the Radiation Field(98% complete; additional material may be added)
5.2 Terms of Radiative Transfer
5.3 The Transfer Equation
5.4 Applying the Transfer Equation
Chaper 6: Gas Physics and Ionzation Processes
6.1 Velocity and Speed Distributions(20% complete; currently working on this one)
6.2 Mean Kinetic Energy of Particles
6.3 Gas Pressure
6.4 Gas Dynamics
6.5 Thermodynamic Equilibrium
6.6 The Ultraviolet Background Radiation
6.7 Photoionization Balancing
6.8 Collisional Ionization Balancing
6.9 Heating and Cooling
Chaper 7: Cross Sections
7.1 Absorption, Scattering, and Emission(90% complete; currently finishing this one)
7.2 The Monochromatic Plane Wave
7.3 Defining Cross Sections
7.4 The Classical Oscillator
7.5 Atomic Bound-Bound Absorption
7.6 Atomic Continuum Asbsorption
7.7 Scattering Cross Sections
7.8 The Total Exctinction Coefficient
7.9 Recombination
7.10 The Total Emission Coefficient
Chaper 8: Absorption Spectral Features
8.1 Thermal Broadening(90% complete)
8.2 The Voigt Profile
8.3 Equivalent Widths: The Curve of Growth
8.4 Rest-frame Equivalent Widths
8.5 Ionization Edges: The Lyman Break
8.6 Absorption Line Systems
Chaper 9: Spectrographs
9.1 The Spectrograph(100% complete)
9.2 Diffraction Gratings
9.3 Low Order Spectrographs
9.4 Echelle Spectrographs
9.5 Monochromatic Resolving Power
9.6 Spectral Purity
9.7 Instrumental Spread Function (ISF)
9.8 ISF Convolution
9.9 Pixelization
Chaper 10: Spectroscopic Data
10.1 Low versus High Resolution(100% complete)
10.2 Charged Couple Devices
10.3 Reducing the Data Suite
10.4 Extracting the Spectrum
10.5 Wavelength Zero Point
10.6 Flux Calibration
10.7 Continuum Fitting
10.8 Combining Spectra
10.9 Signal-to-Noise Ratio (SN)
10.10 Exposure Times and SN
10.11 Magnitudes
10.12 The K-Correction
Chaper 11: Analysis of Quasar Spectra
11.1 Objective Feature Finding(95% complete)
11.2 Equivalent Width Limits
11.3 Gaussian Profile Fitting
11.4 Identifying Absorption Systems
Chaper 12: Analysis of High Resolution Spectra
12.1 Velocity Resolution(80% complete)
12.2 Complexity of Absorption Systems
12.3 Analysis of Associated Transitions
12.4 Velocity Moments
12.5 Apparent Optical Depth (AOD) Spectra
12.6 AOD Analysis
12.7 Voigt Profile Decomposition
12.8 Pixel Statistics Analysis
Chaper 13: Statistical Analysis of Absorbers
13.1 Surveys(100% complete)
13.2 Redshift Path Sensitivity Function
13.3 Redshift Number Density
13.4 Sizes of Absorbers
13.5 Equivalent Width Distribution
13.6 Two-Point Velocity Clustering
13.7 Mean Gas Density
Chaper 14: Modeling Absorbers
14.1 Photoionization Modeling(50% complete)
14.2 Collisional Ionization Modeling
Chaper 15: The Universe of Absorbers
15.1 The Gunn-Peterson Trough(20% complete)
15.2 Lyman Leaks and Reionization
15.3 The Proximity Effect
15.4 The Lyman Alpha Forest
15.5 The He II Forest
15.6 The Lyman Limits Systems (LLS)
15.7 Galaxy Halos
15.8 The Damped Lyman Alpha Systems (DLAs)