
At a Glance
360 Pages
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Preface | p. xi |
Astronomical sources | p. 1 |
The electromagnetic spectrum | p. 1 |
Several astronomies | p. 4 |
Thermal radiation from an ideal source | p. 6 |
Dilute radiation | p. 7 |
Stars | p. 8 |
Magnitudes | p. 11 |
Magnitude systems | p. 13 |
Inverse square law | p. 13 |
Interstellar dust | p. 15 |
Absolute magnitudes and colour excess | p. 16 |
Bolometric magnitudes and bolometric corrections | p. 19 |
Surface photometry | p. 19 |
The estimation of absolute magnitude | p. 20 |
Nebulae and high temperature plasmas | p. 22 |
Thermal radiation | p. 22 |
Emission lines | p. 25 |
Non-thermal radiation | p. 26 |
Synchrotron radiation | p. 26 |
Inverse Compton scattering | p. 27 |
Cerenkov radiation | p. 28 |
The Zeeman effect | p. 29 |
Observational limits | p. 31 |
Coherence | p. 31 |
Coherence time and length | p. 34 |
Photon flux | p. 35 |
Photon noise | p. 35 |
Wave noise | p. 37 |
Detection | p. 40 |
Incoherent detection | p. 40 |
Coherent detection | p. 41 |
Detection limits | p. 42 |
Optical | p. 42 |
Infrared and radio | p. 45 |
Fluxes and limit estimates in janskys | p. 46 |
Air mass | p. 46 |
Optical extinction by the atmosphere | p. 47 |
Atmospheric transparency at radio frequencies | p. 50 |
Sky brightness | p. 51 |
Radio sky brightness | p. 52 |
Celestial coordinates | p. 53 |
Precession | p. 54 |
Julian Day | p. 55 |
Proper motion | p. 56 |
Aberration of starlight | p. 56 |
Astrometric precision and astrometric catalogues | p. 57 |
Doppler shift, radial velocity | p. 60 |
Autocorrelation techniques | p. 61 |
Precise differential radial velocities | p. 62 |
Radio frequency radial velocities | p. 63 |
Red shift and the K correction | p. 63 |
Red shift from colour | p. 64 |
Barycentric and heliocentric corrections | p. 64 |
Telescopes | p. 66 |
Single telescopes | p. 66 |
Gamma-ray telescopes - Cos-B | p. 66 |
Non-focussing collimators | p. 70 |
Phased arrays | p. 75 |
Pencil beam interferometers | p. 78 |
Reflecting telescopes | p. 79 |
Telescope exit pupil | p. 82 |
Reflectivity | p. 83 |
Grazing incidence optics | p. 85 |
Oblique aberrations | p. 91 |
Schmidt telescopes | p. 93 |
Ritchey--Chretien telescopes | p. 101 |
Instrument adaptors/offset guiders | p. 105 |
Infrared telescopes | p. 105 |
Coude focus | p. 109 |
Telescope flexure | p. 111 |
Induced polarisation | p. 114 |
Optical fibres | p. 115 |
Refracting telescopes | p. 116 |
Telescope orientation | p. 117 |
Atmospheric refraction | p. 118 |
Optical apodisation and the tapering of radio antenae | p. 120 |
Optical apodisation | p. 120 |
Tapering of radio antennae and feed horns | p. 122 |
Seeing, speckles, and scintillation | p. 125 |
Modulation (MTF) and optical transfer functions (OTF) | p. 125 |
Telescope transfer function and atmospheric transfer function | p. 126 |
Optimum sampling | p. 127 |
Atmospheric turbulence | p. 130 |
Speckles | p. 131 |
Speckle interferometry | p. 132 |
Amplitude interferometry | p. 136 |
Seeing | p. 137 |
Scintillation | p. 139 |
Optical image profiles (long exposure OTF) | p. 140 |
Choice of optical telescope sites | p. 141 |
Seeing compensation techniques | p. 144 |
Scintillation at radio frequencies | p. 146 |
Ionospheric birefringence | p. 150 |
Spectrographs | p. 151 |
Grating spectrographs | p. 151 |
Efficiency in the presence of seeing | p. 151 |
Image slicers | p. 154 |
Extended sources | p. 155 |
Spectral resolution and grating characteristics | p. 156 |
Echelle spectrographs | p. 160 |
X-ray and infrared | p. 162 |
Wide field spectroscopy | p. 164 |
Objective prism, grism, and grens | p. 164 |
Aperture plates | p. 165 |
Fabry--Perot interferometers | p. 169 |
Michelson interferometer | p. 172 |
The Fellgett and multiplex advantages | p. 175 |
The Jaquinot advantage | p. 176 |
Autocorrelation spectroscopy at radio frequencies | p. 177 |
Dilute apertures | p. 179 |
The interplanetary gamma-ray burst network | p. 179 |
Two-beam interferometry | p. 180 |
Intensity interferometry | p. 180 |
The Michelson stellar interferometer | p. 186 |
Optical | p. 186 |
Infrared incoherent detection | p. 189 |
Infrared coherent detection | p. 191 |
Radio interferometers | p. 193 |
Long baseline interferometry | p. 195 |
Aperture synthesis | p. 198 |
The very large array | p. 204 |
Occultations | p. 207 |
Lunar occultations | p. 207 |
X-ray | p. 209 |
Optical and infrared | p. 210 |
Radio | p. 212 |
Single channelled detectors | p. 216 |
Incoherent detection | p. 216 |
Responsive quantum efficiency (RQE) | p. 216 |
RQE enhancement | p. 218 |
Detective quantum efficiency (DQE) | p. 218 |
Analogue integration | p. 219 |
Photon counting | p. 220 |
Pile-up errors | p. 220 |
The silicon diode: an analogue detector | p. 220 |
Reset (KTC) noise | p. 221 |
Dark noise | p. 222 |
The photomultiplier: a photon counting detector | p. 223 |
Dark noise | p. 226 |
DQE of a photon counting photomultiplier system | p. 228 |
A photoelectric photometer | p. 230 |
Photometric observations | p. 231 |
Monochromators | p. 231 |
Absorption filters | p. 232 |
Interference filters | p. 233 |
Photometric errors from out-of-band radiation | p. 235 |
Polarimetry | p. 239 |
Gamma-ray and X-ray detectors | p. 242 |
Infrared detectors | p. 244 |
Noise in semiconductors | p. 245 |
Noise equivalent power (NEP) | p. 246 |
Thermal detectors | p. 247 |
Photoconductive detectors | p. 248 |
Photovoltaic detectors | p. 250 |
Background radiation | p. 250 |
Signal-to-noise and DQE | p. 254 |
Coherent detection | p. 254 |
Radio receivers | p. 254 |
Infrared heterodyne | p. 257 |
Multi-channelled incoherent detectors | p. 260 |
Photographic emulsion plus microdensitometer | p. 260 |
The photographic process | p. 260 |
Microdensitometer/microphotometers | p. 261 |
DQE of photographic emulsions | p. 265 |
Hypersensitising | p. 267 |
Photographic enhancement and unsharp masking | p. 268 |
Photographic emulsion plus image intensifier | p. 273 |
Magnetically focussed intensifiers | p. 276 |
Electrostatically focussed intensifiers | p. 276 |
Proximity focussed intensifiers | p. 277 |
Coupling of phosphor output and detector | p. 279 |
Electronography | p. 281 |
Signal generating detectors | p. 284 |
Analogue and photon counting television cameras | p. 284 |
The SEC vidicon, a 2D analogue integrating detector | p. 285 |
Photon counting television systems | p. 287 |
The silicon diode, SIT, and ISIT vidicons | p. 288 |
Image tube scanner (ITS) | p. 289 |
Finding and guiding | p. 289 |
Limitations of television cameras | p. 289 |
Solid state detectors | p. 290 |
Self-scanned silicon diode arrays (Reticon) | p. 290 |
Analogue integration | p. 293 |
Photon counting | p. 294 |
The digicon | p. 296 |
Charge transfer devices | p. 297 |
Analogue integration | p. 299 |
CID | p. 299 |
CCD | p. 300 |
Photon counting | p. 307 |
Multi-anode, resistive anode, and microchannel arrays | p. 307 |
Resistive anode MCP | p. 307 |
The microchannel array (MAMA) detector | p. 309 |
Effect of cosmic rays | p. 309 |
Photon counting vs. integration for visible detectors | p. 311 |
High resolution imaging X-ray detector (HRI) | p. 315 |
SI Units and symbols | p. 317 |
Errors of observation | p. 319 |
References | p. 321 |
Index | p. 342 |
Table of Contents provided by Syndetics. All Rights Reserved. |
ISBN: 9780521339070
ISBN-10: 0521339073
Published: 20th April 1987
Format: Paperback
Language: English
Number of Pages: 360
Audience: Professional and Scholarly
Publisher: Cambridge University Press
Country of Publication: GB
Dimensions (cm): 24.7 x 17.4 x 1.9
Weight (kg): 0.62
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