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. 35 |
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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