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| Preface | p. xi |
| Light | p. 1 |
| The story | p. 1 |
| The evidence: astronomical data | p. 3 |
| Models for the behavior of light | p. 6 |
| Measurements of light rays | p. 13 |
| Spectra | p. 16 |
| Magnitudes | p. 26 |
| Summary | p. 31 |
| Exercises | p. 32 |
| Uncertainty | p. 35 |
| Accuracy and precision | p.... MORE |
| Populations and samples | p. 41 |
| Probability distributions | p. 47 |
| Estimating uncertainty | p. 51 |
| Propagation of uncertainty | p. 53 |
| Additional topics | p. 56 |
| Summary | p. 56 |
| Exercises | p. 57 |
| Place, time, and motion | p. 60 |
| Astronomical coordinate systems | p. 61 |
| The third dimension | p. 77 |
| Time | p. 83 |
| Motion | p. 88 |
| Summary | p. 93 |
| Exercises | p. 95 |
| Names, catalogs, and databases | p. 98 |
| Star names | p. 99 |
| Names and catalogs of non-stellar objects outside the Solar System | p. 108 |
| Objects at non-optical wavelengths | p. 112 |
| Atlases and finding charts | p. 112 |
| Websites and other computer resources | p. 114 |
| Solar System objects | p. 114 |
| Summary | p. 116 |
| Exercises | p. 117 |
| Optics for astronomy | p. 118 |
| Principles of geometric optics | p. 118 |
| Lenses, mirrors, and simple optical elements | p. 127 |
| Simple telescopes | p. 135 |
| Image quality: telescopic resolution | p. 137 |
| Aberrations | p. 143 |
| Summary | p. 154 |
| Exercises | p. 155 |
| Astronomical telescopes | p. 157 |
| Telescope mounts and drives | p. 157 |
| Reflecting telescope optics | p. 160 |
| Telescopes in space | p. 168 |
| Ground-based telescopes | p. 175 |
| Adaptive optics | p. 180 |
| The next stage: ELTs and advanced AO | p. 190 |
| Summary | p. 192 |
| Exercises | p. 193 |
| Matter and light | p. 196 |
| Isolated atoms | p. 196 |
| Isolated molecules | p. 204 |
| Solid-state crystals | p. 205 |
| Photoconductors | p. 218 |
| The MOS capacitor | p. 219 |
| The p--n junction | p. 221 |
| The vacuum photoelectric effect | p. 227 |
| Superconductivity | p. 229 |
| Summary | p. 232 |
| Exercises | p. 233 |
| Detectors | p. 235 |
| Detector characterization | p. 236 |
| The CCD | p. 243 |
| Photo-emissive devices | p. 260 |
| Infrared arrays | p. 265 |
| Thermal detectors | p. 269 |
| Summary | p. 272 |
| Exercises | p. 273 |
| Digital images from arrays | p. 275 |
| Arrays | p. 275 |
| Digital image manipulation | p. 281 |
| Preprocessing array data: bias, linearity, dark, flat, and fringe | p. 286 |
| Combining images | p. 297 |
| Digital aperture photometry | p. 309 |
| Summary | p. 320 |
| Exercises | p. 321 |
| Photometry | p. 323 |
| Introduction: a short history | p. 323 |
| The response function | p. 326 |
| The idea of a photometric system | p. 336 |
| Common photometric systems | p. 337 |
| From source to telescope | p. 344 |
| The atmosphere | p. 350 |
| Transformation to a standard system | p. 360 |
| Summary | p. 363 |
| Exercises | p. 364 |
| Spectrometers | p. 368 |
| Dispersive spectrometry | p. 369 |
| Dispersing optical elements | p. 371 |
| Spectrometers without slits | p. 380 |
| Basic slit and fiber spectrometers | p. 382 |
| Spectrometer design for astronomy | p. 385 |
| Spectrometric data | p. 393 |
| Interpreting spectra | p. 399 |
| Summary | p. 402 |
| Exercises | p. 404 |
| Appendices | p. 407 |
| References | p. 437 |
| Index | p. 441 |
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