- Introduction
- The quantum nature of light
- Photometric concepts and radiometric quantities
- General definitions
- Spectral or monochromatic quantities
- Usages in engineering and astrophysics
- Point sources and extended sources
- Natural sources of diffuse illumination
- Detectors
- The ideal detector
- The common detector and its characteristic parameters
- Geometrical properties
- Spectral and dynamical properties
- Temporal properties
- Noise
- The most versatile detector of light images
- Ancient catalogue
- Definition of the magnitude scale
- The perception of colors
- Colors and visual observations
- Major sources of errors in ancient visual observations
- Magnitude
- Magnitude systems
- Bolometric magnitude
- Apparent and absolute magnitudes
- Color index
- Characteristics of the photometric response curve
- The telescope
- Types
- Requirements and specifications
- F-ratio
- Scale in the focal plane
- Size of the telescope
- Stability of mount
- Accuracy of tracking
- Traking of moving objects
- Setting
- Offset guiding
- Optics
- Automated versus manuel telescopes
- Photoelectric photometers
- Types of photoelectric photometers
- The sequential photometer
- The simultaneous photometer
- The multi-star photometer
- The photomultiplier
- The photoelectric effect
- Types of photomultipliers
- The essential parts of a photomultiplier tube
- The glass housing
- The photocathode
- The dynodes
- Anode current and its measurement
- Characteristics of photomultipliers
- Sensitivity, amplification and drift
- Dark current
- Dead time
- Photometric filters
- Fundamental characteristics
- Gelatin filters
- Glass filters
- Interference filters
- Custom-design filters
- Image-quality filters
- Neutral-density filters
- Circular variable filters
- Atmospheric extinction
- Absorption, scattering and dispersion of light
- Monochromatic extinction
- Definition of the air mass
- Calculation of the air mass
- Heterochromatic extinction
- Second-order coefficient
- A rigorous second-order method
- Conclusions
- Atmospheric turbulence: scintillation and seeing
- Scintillation
- Seeing
- Color transformation
- Introduction
- Narrow-band photometry
- Blackbody radiation
- Other spectral distributions
- The general color-transformation problem
- Interstellar extinction
- Monochromatic extinction
- Reddening vector
- Color excess
- Reddening-free indices
- Wide-band extinction
- Principle of data analysis
- Introduction
- Old or new style reductions
- Fitting a model
- Monochromatic photometry
- The multi-night technique: an intuitive view
- The simplest multi-night case
- Bouguer's law for several stars
- Variable extinction
- Unstable instrumentation
- Normalization to a standard scale
- On the meaning of the function phi
- Multifilter photometry
- Narrow-band multifilter photometry
- Color transformations
- Wide-band multifilter photometry
- Fractioning the standard set
- Diaphram effects
- Bright and faint stars
- General remarks
- Examples of reduction algorithms
- Homogenization
- Introduction
- Conformity
- Homogenization
- Merging data from a simple system
- Conclusions
- Infrared photometry
- Introduction
- Chopping and nodding
- The detector
- The photometer
- Observation and reduction of infrared data
- Day-time observing
- Charge-coupled devices
- Introduction
- The detector
- The camera
- Characteristics of CCDs
- Extraction of data from a frame
- Aperture photometry
- Profile fitting
- The point-spread function
- Analytic or empirical PSF
- Stellar photometry using the PSF
- Extinction
- Color transformation
- Photographic photometry
- Introduction
- The photographic emulsion as a storage medium
- The characteristic curve
- Post-observational processing of plates and films
- Calibration of digitally recorded photographic densities
- Photometric analysis of photographic intensities
- The observations
- Introduction
- Preparing the observing run
- Feasibility of the programme
- Programme scheduling
- Absolute photometry
- Differential photometry
- Spurious frequencies
- Evaluation of the quality of the signal for non-imaging
detectors
- Noise and error on sky background
- Some pratical hints
- Instrument checking
- Control of seeing
- Sky background measurements
- Focal-plane diaphragm
- Front diaphragm
- Dead time
- Photometric systems
- Introduction
- The visual system
- Photographic systems
- Photoelectric systems
- The Johnson-Morgan UBV(RI)
- The infrared JHKLM system
- The Geneva UBVB1 B2 V1 G system
- The Walraven VBLUW system
- The Stromgren ubvy Beta system
- H alpha systems
- The WF/PC filter system of the Hubble Space Telescope
- The IHW filter system for cometary research
- Absolute calibration
- Appendix A. References
- Appendix B. Glossary
- Appendix C. Symbols and notations
- Appendix D. Index