Next: 18.2 ALMA Up: 18 Language: CLEAN\ Internal Help Previous: 18 Language: CLEAN\ Internal Help Contents Index
The CLEAN\ Language contains commands related to UV data handling, UV to DataCubes conversion and DataCube processing.
ALMA : Joint deconvolution of ALMA and ACA dirty images
BUFFERS : List and Display the known buffer status
CCT_CLEAN : Compute CLEAN image from Clean Component Table, without residuals
CCT_CONVERT : Convert an image into a Clean Component Table
CCT_MERGE : Merge two Clean Component Tables
CLEAN : Deconvolve a dirty image using the current METHOD
DISCARD : Discard one of the active data buffers
DUMP : Dump the control parameters of the deconvolution algorithms
FIT : Fit the dirty beam
LOG : LOG "command argument" B|F|S
MAP_CONVOLVE : Spatially Smooth a data Cube
MAP_COMBINE : Combine two data Cubes
MAP_COMPRESS : Average a Cube by several channels
MAP_INTEGRATE : Compute a Moment 0 Map
MAP_REPROJECT : Spatial resampling of a Cube
MAP_RESAMPLE : Resample a Cube on a different Velocity/Frequency scale
MAP_SMOOTH : Smooth by N channels
MOSAIC : Change the mosaic processing mode
MX : Iteratively image and deconvolve a dirty image
PRIMARY : Apply primary beam correction
READ : Read the input files in internal buffers
SPECIFY : Change Frequency / Velocity /Unit scale or the Telescope
SUPPORT : Define the support used to search clean components
UV_BASELINE : Subtract a continuum baseline from a Line UV data
UV_CHECK : Check UV data for null visibilities or per channel flags.
UV_COMPRESS : Compress a Line UV data into another Line UV data
UV_CONTINUUM : Compress a Line UV data into a Continuum UV data
UV_EXTRACT : Extract a range from
UV_FILTER : Filter out (line) channels
UV_FLAG : Interactively flag UV data
UV_MAP : Build the dirty image and beam from a UV table
UV_RESAMPLE : Resample (in Velocity) the UV data
UV_RESIDUAL : Subtract Clean Component from the UV Data
UV_RESTORE : Restore a Clean image from UV data and Clean Components
UV_REWEIGHT : Evaluate UV weights from visibility statistics
UV_SHIFT : Shift a UV table to common phase center
UV_SMOOTH : Smooth spectrally a Line UV data
UV_SPLIT : Split a UV table into Line and Continuum
UV_STAT : Gives beam sizes and noise properties as a function of
tapering or robust weighting parameter
UV_SUBTRACT : Subtract Continuum visibilities from Line UV data
UV_TIME : Time average the current UV data
UV_TRIM : Suppress useless information from UV data
UV_TRUNCATE : Truncate the baseline range of the UV data
WRITE : Save internal buffers or Image variables onto output files