Observational Astrophysics
P. Lena, F. Lebrun & F. Mignard (2nd edition, Springer, 1998)
- Chapter 1, Introduction and Section 1.1 (astrophysical information carriers)
- Chapter 1, Section 1.2 (properties of photons and electromagnetic waves)
- Chapter 3, Introduction and Section 3.1 (radiation quantities)
- Chapter 3, Section 3.2.1 (blackbody radiation)
- Chapter 3, Section 3.3 (magnitudes)
- Chapter 2, Introduction and Section 2.1 (effects and structure of atmosphere)
- Chapter 2, Section 2.2 (atmospheric absorption)
- Chapter 3, Section 3.4 (photometry through the atmosphere)
- Chapter 2, Section 2.3 (atmospheric emission)
- Chapter 2, Section 2.4 (atmospheric scattering)
- Chapter 2, Section 2.5 (atmospheric refraction and dispersion)
- Chapter 2, Section 2.6, only qualitatively (atmospheric turbulence)
- Chapter 2, Section 2.7 (ground-based observing sites)
- Chapter 2, Section 2.8 and 2.9 (observing from space)
- Appendix A (basic Fourier theory)
- Chapter 4, Introduction and Section 4.1 (Imaging through geometrical optics)
- Chapter 4, Section 4.2.3 (Imaging through wave optics)
- Chapter 4, Introduction Section 4.3 (Telescopes in practice)
- Chapter 4, Section 4.3.2 and 4.3.3 until Michelson Interferometry (p. 150) (Large telescopes)
- Chapter 4, Section 4.3.4 (Space telescopes)
- Chapter 4, Section 4.3.5 and 4.3.6 (X-ray and gamma-ray telescopes)
- Chapter 4, Section 4.4 Introduction (seeing)
- Chapter 4, Section 4.4.1 and 4.4.2 (mathematics of seeing)
- Chapter 4, Section 4.4.4 (adaptive optics)
- Chapter 5, Introduction (spectroscopy)
- Chapter 5, Section 5.2 (spectral data)
- Chapter 5, Section 5.3 Introduction and Section 5.3.1 (figures of merit)
- Chapter 5, Section 5.3.3 until Multi-Object Spectroscopy (p. 226) (grating spectrographs,
echelles)
- Chapter 5, Section 5.3.3 from Multi-Object Spectroscopy (p. 226) until The Spectroheliograph (p. 230) (multiplexing with grating spectrographs)
- Chapter 5, Sections 5.3.2 and 5.3.5 (interference filters,
Fabry-Perot spectrometers)
- Chapter 5, Section 5.3.4 except The Holographic Fourier Spectrometer (p. 235) (Fourier Transform Spectrograph)
- Appendix B, Section B.1 (random variables)
- Chapter 6, Section 6.1.3 (random variables and sampling)
- Appendix B, Section B.2, only Poisson process (p. 245-246) (photon stream as Poisson process)
- Chapter 6, Introducion, Sections 6.1.1 and 6.1.2 and 6.2.1 (NEP and NEFD)
- Chapter 7, Introducion and Section 7.1 (detector characterisctics)
- Chapter 7, Section 7.2 Introduction (photon detection methods)
- Chapter 7, Section 7.2.1 until extrinsic photoconductor (p. 301) (intrinsic photoconductors)
- Chapter 7, Section 7.2.1 from extrinsic photoconductor (p. 301) until photovoltaic effect (p. 303) (extrinsic photoconductors)
- Chapter 7, Section 7.2.1 from photovoltaic effect until quantum wells (p. 303) (photovoltaic detectors)
- Chapter 7, Section 7.2.1 from thermal effects (p. 308) and Section 7.3.5 from bolometers (p. 343) (bolometers)
- Chapter 7, Section 7.2.1 from photochemical effect until photoionization of gases (p. 304) and Section 7.3.1 (photographic plates)
- Chapter 7, Section 7.3.3 until infrared solid-state imagers (p. 332) except the reticon (p. 326) and Section 7.3.1 (CCDs)
- Chapter 7, Section 7.3.3 from infrared solid-state imagers (p. 332) except detectors coupled to a CCD (p. 333) (infrared arrays)
- Chapter 6, Section 6.2 until quantum noise (Section 6.2.1) (incoherent vs. coherent detection)
Electronic imaging in astronomy
I. McLean (Wiley, 1997)
- Chapter 10, Sections 10.3 through 10.5 (properties of arrays)
- Chapter 10, Section 10.9 (S/N ratio of detectors with readout noise)
Tools of radio astronomy
K. Rohlfs & T.L. Wilson (2nd edition, Springer, 1996)
- Chapter 1, Sections 1.1 through 1.5 (Rayleigh-Jeans approximation and brightness temperature)
- Chapter 1, Section 1.6 (Nyquist theorem and noise temperature)
- Chapter 4, Section 4.2.2 (only the result) (radiometer equation)
- Chapter 4, Section 4.2.3 until table 4.2 (p. 67) (receiver stability)
- Chapter 8, Section 8.4.4 (switching techniques)
- Chapter 4, Section 4.2.1 (minimum noise of a coherent system)
- Chapter 4, Section 4.3.2 Introduction and Sections 4.3.2.1 and 4.3.2.2 (receiver components)
- Chapter 4, Section 4.3.2.3 (mixers)
- Chapter 4, Section 4.6 Introduction (local oscillators)
- Chapter 4, Section 4.4.5 Introduction and Sections 4.4.5.1 and 4.4.5.3 (mixer implementation)
- Chapter 4, Section 4.4.5.2 (amplifiers)
- Chapter 4, Sections 4.6.1 and 4.6.3 (principle only) (filter bank and acousto-optical spectrograph)
- Chapter 4, Section 4.6.2 and its subsections (no proofs) (autocorrelator spectrograph)
- Chapter 5, Section 5.5 Introduction and Sections 5.5.1 and 5.5.2 (antenna pattern)
- Chapter 5, Section 5.5.3 (aperture efficiency)
- Chapter 5, Section 5.5.4 (antenna temperature and brightness temperature)
- Chapter 8, Sections 8.2.1, 8.2.2 and 8.2.3 (main beam brightness temperature)
- Chapter 6, Sections 6.2 and 6.3 (antennas and Fourier optics)
- Chapter 6, Section 6.4 (feeds and focal arrangements)
- Chapter 6, Sections 6.5 (qualitative) and 6.6 (dish surface properties)
- Chapter 7, Section 7.1 (introduction to aperture synthesis)
- Chapter 7, Section 7.4 until In order to understand (P. 167) (adding and correlating interferometers)
- Chapter 7, Section 7.4 from In order to understand (P. 167) (interferometer response)
- Chapter 7, Section 7.5 (aperture synthesis)
- Chapter 7, Section 7.8 (VLBI)
- Chapter 7, Section 7.7 (synthesized beam)
- Chapter 8, Section 8.5 Introduction and Sections 8.5.1 and 8.5.3 (deconvolution)
- Chapter 8, Section 8.5, Section 8.5.5 (self-calibration)
Paul van der Werf (pvdwerf@strw.leidenuniv.nl)
Last modified: Mon Apr 17 22:19:12 2000