Tables. Appendix G. Instrumental characteristics. References.. From stars to galaxies. Part 1: light. Astronomy and Astrophysics Library. Edited by E. Contini. Berlin Heidelberg: Springer. Astrophysics and Space Science Library. Springer; doi:10.1007/978-3-642-05726-7. 1 7.5-inch Andru Campbell Telescope (AST). Abbreviation: Andru. 1.9-metre Anglo-Australian Telescope (AAT). Abbreviation: AAT. Abbreviation: AU. 2.5-metre Automatic Photographic Telescope (APT). Abbreviation: APT. Abbreviation: AU. 3.5-metre Isaac Newton Telescope (INT). Abbreviation: INT. Abbreviation: AU. 4.2-metre Mount Stromlo Telescope (MST). Abbreviation: MST. Abbreviation: AU.
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List of figures
Fig. 1 The plan of the light source showing the path of the light (A); the path of the diffused light (B); the path of the light reflected by the translucent screen (C); and the path of the light reflected by the opaque screen (D).
Fig. 2 Diagram of an optical system.
Fig. 3 The telescope.
Fig. 4 The detector.
Fig. 5 Schematic diagram showing the relation between the size of the aperture of the system, the rays that can be observed, the intensity of the stars, the effect of atmospheric scattering, the amount of dispersion due to the atmosphere, and the size of the pupil.
Fig. 6 The diagram of the image of the entrance pupil with the rays that go to the sensor and the size of the image.
Fig. 7 Diagram of the image of the entrance pupil with the rays that go to the sensor and the size of the image.
Fig. 8 The image of the entrance pupil.
Fig. 9 The intensity of the stars.
Fig. 10 The diagram of the sensor and the intensity of the star (not observed).
Fig. 11 The light coming out from the telescope.
Fig. 12 The intensity of the flux of the star.
Fig. 13 The intensity of the flux coming out from the telescope.
Fig. 14 The diagram of the
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