Key concepts
The following is a list of common terms used in the radio astronomy domain. Key concepts that form the ubiquitous language for starbox have links with further details. This is a living document and will be updated as code is added.
Observations
- Observation
- Scan: A contiguous time interval during which the telescope observes a single field with fixed pointing.
- Calibrator: A source observed primarily to estimate instrumental or propagation effects.
- Target: A source or field observed for scientific analysis.
Pointing
- Pointing
- Right ascension
- Declination
- Hour angle
- Integration time
- Phase centre
Sky and signals
- Polarization
- Faraday rotation
- RFI
- [Sources]: sources of radio emission in a sky model or image.
- Point source
- Extended source (extended emission or gaussian blob)
- Sky model (source catalog, source list)
- Apparent sky: The sky brightness distribution as modified by instrumental and propagation effects.
- True sky: The intrinsic sky brightness distribution, independent of the instrument.
- Patches: Groups of sky model components treated together, typically for direction-dependent calibration.
Modes
- Wideband
- Widefield
- Drift scan
Units & quantities
- Jansky
- Flux density (flux, intensity or brightness)
Coordinates & axes
- Direction cosines (l,m,n)
- Baseline coordinates (u,v,w)
Telescope
- Telescope (interferometer, array, sub-array, station, sub-station)
- Antenna (receptor, receiver)
- Aperture
Array configuration
- uv-coverage
- Baseline
- Rigid rotation
Interferometry
- VLBI
- Aperture synthesis
- Fringes
- Correlator
- Delay
Data processing
Beam
- Beam model (primary beam)
- Beam forming
- Tied-array beam forming
- Side lobes
Calibration
- Calibration solution (solution): An estimated set of parameters that can be applied to visibilities to correct for corruptions introduced by the hardware, electronics, atmosphere or thermal noise.
- Reference antenna: A station used to fix phase and amplitude degeneracies during calibration.
- Calibration: The process of estimating and applying calibration solutions.
- Jones matrix
- Solver: The algorithm used to estimate calibration solutions.
- Predict: The process of predicting ideal visibilities from sky model components.
- Self-calibration cycle: An iterative loop of imaging, model update, and calibration.
Modes
- Phase-only
- Amplitude and phase
- Direction-independent
- Direction-dependent
- Self-calibration (self-calibration cycle)
Gains
- Phase
- Amplitude
- Complex gains
Effects
- Corruptions
- Phase screen (TEC screen)
- Bandpass
- Delay
- Direction-dependent effect (DDE)
Control
- Flagging
- Reference antenna
Imaging
Modes
- Continuum imaging
- Spectral imaging
Data products
- Artifacts
- Images
- Dirty image
- Residual image
- Clean image (restored image)
- Model image
- Image cube: one image per frequency channel stacked together.
- Spectral index map
Quality Metrics
- SNR
- Dynamic range
Wide-field
- Facet
- Sector
- Field
- W-term
Polarization
- Stokes parameters (I, Q, U, V)
Deconvolution
- Deconvolution
- Briggs weighting
- Model component (CLEAN component)
- Major cycle
- Minor cycle
- Point spread function (PSF)
- FWHM
- First null
Concepts
- Image plane (image space, pixel space)
- Visibility plane (visibility space, Fourier space)
Data formats
- Measurement set
- FITS file
- CASA table
- h5parm
Algorithms
- W-stacking
- CLEAN
- Högbom CLEAN
- Multi-scale CLEAN
- Radio Interferometry Measurement equation (RIME)
- Gridding
- Source finding