Astronomical Spectrographs and their History
, by John Hearnshaw- ISBN: 9780521882576 | 0521882575
- Cover: Hardcover
- Copyright: 2/23/2009
Preface | p. ix |
Acknowledgements | p. xi |
The historical development of astronomical spectroscopes and spectrographs | p. 1 |
Colour, refrangibility and wavelength | p. 1 |
The refraction of light | p. 1 |
Wavelength, colour and spectral lines | p. 2 |
The collimator in prism spectroscopes | p. 2 |
Some notable astronomical prism spectroscopes of the mid nineteenth century | p. 3 |
Improvements in prism spectroscope design in the later nineteenth century | p. 5 |
Spectroscope slits | p. 10 |
Projected scales and automatic line recorders | p. 10 |
The development of the prism spectrograph | p. 11 |
The spectrographs of Henry Draper and William Huggins | p. 11 |
Further prism spectrographs: Potsdam, Paris and Lick | p. 13 |
The development of the diffraction grating | p. 17 |
Grating mountings for laboratory and astronomical spectrographs | p. 24 |
Concave grating mountings | p. 25 |
Early grating spectroscopes and spectrographs | p. 29 |
Early solar grating spectroscopy | p. 29 |
Stellar grating spectroscopy before 1900 | p. 30 |
Astronomical grating spectrographs and their development from 1900 | p. 31 |
Prism spectrographs in the twentieth century | p. 36 |
References | p. 42 |
The theory of spectroscopes and spectrographs | p. 46 |
General properties of a spectrograph | p. 46 |
The spectrograph figure of merit | p. 46 |
Resolving power and throughput of prism instruments | p. 48 |
Dispersive properties of prisms and the diffraction-limited resolving power | p. 48 |
Slit-limited resolving power of prism spectrographs | p. 50 |
Properties of glasses used in prisms | p. 52 |
Prism spectrograph throughput | p. 53 |
Figure of merit for prism spectrographs | p. 54 |
Resolving power and throughput of diffraction grating spectrographs | p. 55 |
The diffraction-grating equation and angular dispersion | p. 55 |
Fourier analysis of diffraction gratings | p. 56 |
Diffraction-limited resolving power of a grating | p. 57 |
Slit-limited resolving power of grating spectrographs | p. 58 |
Comparison of the figure of merit of prism and grating spectrographs | p. 60 |
Cameras and detectors: some simple requirements | p. 60 |
Reciprocal dispersion and free spectral range | p. 61 |
Detector resolution and the Nyquist sampling theorem | p. 62 |
Number of detector pixels required | p. 63 |
Grating efficiency, shadowing and the quasi-Littrow angle | p. 63 |
Gratings not illuminated in the normal plane | p. 66 |
The grism as a dispersing element | p. 67 |
Some miscellaneous aspects of spectrograph design | p. 68 |
Baranne's white pupil concept | p. 68 |
Some general principles of spectrograph design | p. 69 |
References | p. 70 |
High resolution spectrographs | p. 72 |
Theory of the coudé spectrograph | p. 72 |
History of the coudé spectrograph | p. 73 |
Early coudé refractors | p. 73 |
Coudé prism spectrographs at Mt Wilson | p. 73 |
The coudé grating spectrograph with Schmidt cameras | p. 74 |
New coudé spectrographs | p. 75 |
The image slicer in high resolution spectroscopy | p. 79 |
Theory of the échelle spectrograph | p. 81 |
Line tilt in échelles | p. 83 |
Efficiency of échelles as a function of ¿ and ¿ | p. 84 |
Historical development of échelle spectrographs | p. 86 |
Coudé échelle spectrographs | p. 86 |
Cassegrain échelle spectrographs | p. 88 |
Fibre-fed échelle spectrographs | p. 88 |
References | p. 93 |
Solar spectrographs and the history of solar spectroscopy | p. 96 |
Spectroscopy of the solar chromosphere | p. 96 |
The discovery of helium | p. 96 |
The structure of prominences revealed | p. 100 |
The measurement of solar spectrum wavelengths | p. 101 |
Solar wavelengths from Fraunhofer's gratings | p. 101 |
Kirchhoff's drawing of the solar spectrum | p. 102 |
New grating measurements from Ångström and others | p. 102 |
Henry Rowland and the concave grating | p. 103 |
The revision of the Rowland scale | p. 105 |
Hale and Deslandres and the spectroheliograph | p. 105 |
Hale and the dedicated solar spectrograph and observatory | p. 113 |
Further developments in solar spectrographs and telescopes | p. 117 |
The work of Francis and Robert McMath | p. 120 |
New innovations in solar spectroscopy, 1940-1965 | p. 121 |
Photoelectric recording of the solar spectrum | p. 121 |
Lead sulphide cells and the solar infrared | p. 122 |
First use of the échelle grating for solar spectroscopy | p. 125 |
Solar ultraviolet spectroscopy from rockets | p. 128 |
The solar vacuum spectrograph | p. 129 |
The double-pass solar spectrograph | p. 131 |
The McMath solar telescope and spectrograph at Kitt Peak | p. 133 |
Concluding remarks on solar spectrographs | p. 136 |
References | p. 136 |
Objective prism spectrographs | p. 140 |
Theory of the objective prism spectrograph | p. 140 |
The history of objective prism spectroscopy | p. 143 |
Objective prism spectroscopy in the nineteenth century | p. 143 |
Objective prism astrographs in the twentieth century | p. 146 |
Spectrophotometry with objective prism astrographs | p. 149 |
Objective prism radial velocities | p. 152 |
Objective prism surveys with Schmidt telescopes | p. 155 |
References | p. 159 |
Ultraviolet and nebular spectroscopy | p. 162 |
Ultraviolet and nebular spectroscopy | p. 162 |
Henry Draper and William Huggins, pioneers in ultraviolet stellar spectroscopy | p. 162 |
Ultraviolet spectrographs at Lick Observatory | p. 164 |
Cameras for nebular and ultraviolet spectrographs | p. 165 |
Nebular slit spectrographs at Yerkes and McDonald observatories | p. 167 |
Ultraviolet spectroscopy with aluminized reflectors and Schmidt cameras | p. 167 |
Ultraviolet spectroscopy from above the Earth's atmosphere | p. 169 |
Some technical aspects of ultraviolet spectroscopy | p. 169 |
Ultraviolet spectroscopy from rockets and balloons | p. 170 |
The Orbiting Astronomical Observatories | p. 175 |
Ultraviolet spectroscopy with Europe's TD-1 satellite | p. 177 |
The International Ultraviolet Explorer | p. 178 |
Ultraviolet spectroscopy from manned spacecraft | p. 179 |
References | p. 182 |
Multi-object spectrographs | p. 184 |
Low resolution multi-object spectroscopy | p. 184 |
Aperture plate multi-object spectroscopy | p. 184 |
Multi-object spectroscopy using optical fibres and aperture plates | p. 185 |
Multi-object spectroscopy with automated fibre positioning | p. 190 |
Spectroscopy with an integral field unit | p. 193 |
References | p. 193 |
Ten pioneering spectrographs of the late twentieth century | p. 195 |
Introduction to spectrographs of the late twentieth century | p. 195 |
The ESO faint object spectrograph and camera: EFOSC | p. 195 |
The Keck High Resolution Echelle Spectrometer: HIRES | p. 196 |
The Keck Low Resolution Imaging Spectrometer: LRIS | p. 200 |
ELODIE at Haute-Provence | p. 201 |
The 2dF spectrographs at the Anglo-Australian telescope | p. 203 |
The Space Telescope Imaging Spectrograph: STIS | p. 205 |
The Ultraviolet Echelle Spectrograph at ESO Paranal: UVES | p. 206 |
The Sloan Digital Sky Survey spectrographs | p. 208 |
The Hercules spectrograph at Mt John | p. 210 |
HARPS, the high accuracy radial-velocity planet searcher | p. 211 |
References | p. 212 |
Figure sources and acknowledgements | p. 214 |
Name index | p. 220 |
Subject index | p. 223 |
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