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Pre-amble
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imager
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imager
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Contents
Pre-amble
IMAGER in short
IMAGER for you...
IMAGER for beginners
IMAGER for previous users of
MAPPING
IMAGER for huge data sets: 100 000 channel imaging with NOEMA or ALMA
IMAGER for lazy or overbooked ones
IMAGER for ALMA data
IMAGER for image analysis and publication plots
IMAGER for Simulations
IMAGER principles
Overview of the data reduction and analysis
The structure of the
IMAGER
program
Fundamental control variable:
BEAM_STEP
–
Read carefully !
Imaging/deconvolution: a brief sequence of commands
Getting Help: the HELP command and the ? token
The input data: UV Tables
In a nutshell
UV table description
NOEMA: UV Tables from CLIC
ALMA: UV Tables from C
ASA
Reading UV tables
UV Table handling
Single-field imaging and deconvolution
In a nutshell
Measurement equation and other definitions
Imaging
Deconvolution
The family of
CLEAN
algorithms (
HOGBOM
,
CLARK
,
MX
,
SDI
,
MRC
,
MULTI
)
Practical advices
Wide-field imaging and deconvolution
In a nutshell
General considerations about wide-field imaging
Mosaicing
Large Mosaics: the
SAULT
method
Mosaic and JvM factor
Short and Zero spacings
In a nutshell
Principle
Algorithms to merge single-dish and interferometer information
Hybridization technique and ALMA
The Zero spacing: an important subset
Short Spacings in practice: command
UV_SHORT
Practical considerations
Mosaic and Self-Calibration
Self Calibration
Self-Calibration in a nutshell
Self-Calibration Principle
Self-Calibration Implementation
Basic use
Advanced use
Transfering the solution to other
uv
data sets.
Data re-weighting
Data flagging
UV plane analysis
Continuum emission
Continuum imaging
Split Continuum and Spectral line imaging
Combined Continuum and Spectral line imaging
The
CONTINUUM
image
Visual Checks and Image Displays
The basic visualization commands
The
VIEWER
program
The
/DIRECTORY
option - Simultaneous display.
Specific
IMAGER
visualisation tools
The Imager PIPELINE tools
Preparing the data
Before using the
PIPELINE
The
PIPELINE
Widget
The non interactive
PIPELINE
User control: the
STOP
symbol
Mosaics and other limitations.
Really Huge Problems
Polarization Handling
Data Handling
The STOKES command
Simulating Observations
Data Analysis
Basic Data Cube Handling and Comparison
Matched Filtering
Line Stacking
Rotationally symmetric structures: Keplerian disks
DISPLAY Language Internal Help
Language
CATALOG
COLOR
COMPARE
EXPLORE
EXTRACT
FIND
INSPECT_3D
LOAD
POPUP
SET
SHOW
SLICE
SPECTRUM
STATISTIC
VIEW
CLEAN Language Internal Help
Language
ALMA
BUFFERS
CCT_CLEAN
CCT_CONVERT
CCT_MERGE
CLEAN
DISCARD
DUMP
FIT
LOG
MAP_CONVOLVE
MAP_COMBINE
MAP_COMPRESS
MAP_INTEGRATE
MAP_REPROJECT
MAP_RESAMPLE
MAP_SMOOTH
SPECIFY
MOSAIC
MX
PRIMARY
READ
SUPPORT
UV_BASELINE
UV_CHECK
UV_COMPRESS
UV_CONTINUUM
UV_EXTRACT
UV_FIELDS
UV_FILTER
UV_FLAG
UV_MAP
UV_RESAMPLE
UV_RESIDUAL
UV_RESTORE
UV_REWEIGHT
UV_SHIFT
UV_SMOOTH
UV_SPLIT
UV_STAT
UV_TIME
UV_TRIM
UV_TRUNCATE
WRITE
UV_TRACKS
CALIBRATE Language Internal Help
Language
APPLY
COLLECT
DERIVE
PLAIT
SCALE_FLUX
MODEL
SOLVE
TRANSFORM
UV_SELF
UV_SELECT
UV_SORT
ADVANCED Language Internal Help
Language
FEATHER
FLUX
HOW_TO
MAP_CONTINUUM
MAP_POLAR
MASK
MFS
MOMENTS
PROPER_MOTION
STOKES
UV_ADD
UV_CIRCLE
UV_CORRELATE
UV_DEPROJECT
UV_FIT
UV_MERGE
UV_MOSAIC
UV_PREVIEW
UV_RADIAL
UV_SHORT
XY_SHORT
BUNDLES Language Internal Help
Language
COMBINE
KEPLER
SELFCAL
SPECTRAL_CLEAN
UV_DETECT
IMAGER Language Internal Help
Language
TIPS
PIPELINE
HOGBOM
CLARK
MRC
MULTISCALE
SDI
SIMULATE
Bugs and Release Notes
Known Bugs
Recent changes in repository
IMAGER versus CASA
Imaging Philosophy and Data Architecture
Frequency and Velocity scales
Transfering UV data from C
ASA
In CASA
In
IMAGER
Transfering Image data
Properties of the Fourier Transform
Revision History
DISPLAY Language
CLEAN Language
ADVANCED Language
CALIBRATE Language
BUNDLES Language
IMAGER Language
SIMULATE Language
References
Index