An introduction to basic practical tools, methods and phenomena that underlie quantitative astronomy.
A Practical Guide to Observational Astronomy
β Scribed by M. Shane Burns
- Publisher
- CRC Press
- Year
- 2021
- Tongue
- English
- Leaves
- 175
- Edition
- 1
- Category
- Library
No coin nor oath required. For personal study only.
β¦ Synopsis
A Practical Guide to Observational Astronomy provides a practical and accessible introduction to the ideas and concepts that are essential to making and analyzing astronomical observations.
A key emphasis of the book is on how modern astronomy would be impossible without the extensive use of computers, both for the control of astronomical instruments and the subsequent data analysis. Astronomers now need to use software to access and assess the data they produce, so understanding how to use computers to control equipment and analyze data is as crucial to modern astronomers as a telescope.
Therefore, this book contains an array of practical problems for readers to test their knowledge, in addition to a wealth of examples and tutorials using Python on the authorβs website, where readers can download and create image processing scripts.
This is an excellent study guide or textbook for an observational astronomy course for advanced undergraduate and graduate astronomy and physics students familiar with writing and running simple Python scripts.
Key Features
- Contains the latest developments and technologies from astronomical observatories and telescope facilities on the ground and in space
- Accompanied by a companion website with examples, tutorials, Python scripts, and resources
- Authored by an observational astronomer with over thirty years of observing and teaching experience
About the Author
M. Shane Burns earned his BA in physics at UC San Diego in 1979. He began graduate work at UC Berkeley in 1979, where he worked on an automated search for nearby supernovae. After being awarded a PhD in 1985, Professor Burns became a postdoctoral researcher at the University of Wyoming. He spent the summer of 1988 as a visiting scientist at Lawrence Berkeley National Lab, where he helped found the Supernova Cosmology Project (SCP). He continued to work as a member of the SCP group while a faculty member at Harvey Mudd College, the US Air Force Academy, and Colorado College. The 2011 Nobel Prize in Physics was awarded to the leader of the SCP for the groupβs "discovery of the accelerating expansion of the Universe through observations of distant supernovae." During his career, Professor Burns has observed using essentially all of the worldβs great observatories, including the Keck Observatory and the Hubble Space Telescope.
β¦ Table of Contents
Cover
Half Title
Title Page
Copyright Page
Dedication
Contents
Preface
CHAPTER 1: Astronomical Coordinates and Time
1.1. HORIZON COORDINATES
1.2. EQUATORIAL COORDINATES
1.3. TELESCOPE MOUNTS
1.4. OTHER COORDINATE SYSTEMS
1.5. TIME IN ASTRONOMY
CHAPTER 2: Optics and Telescopes
2.1. GEOMETRIC OPTICS
2.2. IMAGE SCALE
2.3. RESOLUTION
2.4. TELESCOPE OPTICAL DESIGNS
CHAPTER 3: Measuring Light
3.1. FROM THE STARS TO OUR DETECTOR
3.2. THE MAGNITUDE SYSTEM
3.3. MEASURING MAGNITUDES
3.4. ESTIMATING EXPOSURE TIMES
CHAPTER 4: Charge-Coupled Devices
4.1. LIGHT DETECTION
4.2. CCD READOUT
4.3. DARK CURRENT
4.4. QUANTUM EFFICIENCY
4.5. EXAMPLE CCD CAMERAS
CHAPTER 5: Image Processing
5.1. DISPLAYING IMAGES
5.2. IMAGE ARITHMETIC
5.3. CCD DATA CORRECTION
5.4. COMBINING IMAGES
CHAPTER 6: Photometry
6.1. STANDARD PHOTOMETRIC SYSTEMS
6.2. PHOTOMETRIC DATA REDUCTION
6.3. DIFFERENTIAL PHOTOMETRY
6.4. ABSOLUTE PHOTOMETRY
APPENDIX A: Spherical Trigonometry
APPENDIX B: Data Analysis
B.1. WHAT IS UNCERTAINTY?
B.2. REPORTING UNCERTAINTIES
B.3. ESTIMATING UNCERTAINTIES
B.4. SYSTEMATIC VERSUS RANDOM ERRORS
B.5. STATISTICAL ANALYSIS OF RANDOM ERRORS
B.6. PROBABILITY DISTRIBUTIONS
B.7. PROPAGATION OF UNCERTAINTY
APPENDIX C: Fitting and Graphical Representation of Data
C.1. βA PICTURE IS WORTH A THOUSAND WORDSβ
C.2. DATA FITTING
C.3. LINEAR FITTING
Bibliography
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