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Дата индексирования: Sun Apr 10 12:30:54 2016
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Поисковые слова:
interferometry
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General Information
General Information
Recommended Reading
Acknowledgements
The User Interface
Introduction
The
miriad
Front-End
INP, GO and TASK
HELP
EXIT and QUIT
Command-Line Editing and ER
Interrupting a Task
UNSET
SAVE and LOAD
TPUT and TGET
Summary of
miriad
commands
Miriad
on the World Wide Web
Bug Reports and Giving Feedback
Indirect Parameter Input
Host Command-Line Interface
Writing Shell Scripts
Plotting Concepts
Introduction
The ATNF Visualisation Suite
Using X Windows
PGPLOT Plotting Devices
Miriad
Datasets
Listing Datasets - PRTHD
Inside Datasets
Scratch Files
Miriad
Data Disks at Epping
Visibility Data Concepts
Miriad
Visibility File Format
Miriad
's Calibration Model
On-the-Fly Calibration Correction
Channel Selection, Averaging and Doppler Correction - UV Linetypes
Selecting UV Data in
Miriad
Spectral Window Selection
Selection and Multi-Source/Multi-Frequency Datasets
Polarization/Stokes Handling (stokes and select)
Image Data Concepts
Image Datasets
Image Coordinate Systems
Image Region of Interest (region)
Reduction Strategies
Getting Data In and Out of
Miriad
ATLOD:
Reading RPFITS Files
FITS Tapes and
Miriad
Reading Visibility FITS Files
Information Missing or Incorrect in FITS Files
AIPS Frequency Bugs
Time and FITS Files
Writing Visibility FITS Files
Reading and Writing FITS Images
Archiving and Transporting
Miriad
Datasets
Generating Dummy Visibility Data
Making a Fake Observation
Generating Visibilities from a Model Image
Flagging, Manipulating and Examining Visibility Data
Correcting Visibilites
Initial ``fixes'' to millimetre data
Flagging Visibilities
Interactive Flagging - BLFLAG
Interactive Channel/Baseline Flagging - TVFLAG
Interactive Channel/Baseline Flagging - PGFLAG
General
Miriad
Flagging - UVFLAG
Other Flagging Tasks
AIPS Flagging and
Miriad
- FGFLAG
Flagging Near a Set-Up Change - QVACK
Flagging Based on a Template - UVAFLAG
Flagging a Sector of Data - UVSECTOR
Listing Visibilities
Copying, Concatenating and Averaging Visibility Datasets
Plotting Visibilities
Examining Visibility Variables
Modifying Visibility Datasets
Calibration, the ATCA, and
Miriad
Some Theory
Polarisation
Atmospheric opacity and system temperature
Antenna gain considerations and flux calibration
Instrumental phase
Atmospheric phase and phase calibration considerations
Calibration Methods
Calibration of Data with
XX
,
YY
,
XY
and
YX
Calibration of Data with
XX
and
YY
Only
Determining Calibration Solutions
Determining Gains and Bandpass Functions - MFCAL
Determining Gains and Polarimetric Properties - GPCAL
Copying Calibration Tables - GPCOPY
Displaying Calibration Tables - GPPLT
Deleting Calibration Tables - DELHD
Calibration Strategies
Introduction
Preparing your Data
Calibration
An alternative approach to calibration
Information on planets
The Interpolation Process
Interpolation/Extrapolation Tolerance
Averaging Antenna Gains with Time - GPAVER
Preventing Gain Interpolation - GPBREAK
Interpolation of binned gain solutions
High precision polarimetric calibration
Combining Pre- and Post-August 1994 Data
Imaging
Introduction
Spectral Line Imaging Considerations
Weighting
Computation
Image Deconvolution
Introduction
Deconvolution with CLEAN
The Clark CLEAN
The SDI CLEAN
Region-of-Interest Considerations
The Cotton-Schwab CLEAN
CLEAN Stripes
Computation
Deconvolution with maximum entropy algorithms
Computation
Multi-frequency deconvolution - MFCLEAN
Other deconvolution tasks
Restoring an image
Self-Calibration
Computation
Apply Your Original Calibration Before Self-Calibrating
Self-Calibrating with Multiple Models
Polarisation Handling
Frequency Handling
Multi-Plane Models
Multi-Frequency Models
Input Parameters to the Self-Calibration Tasks
Summary
Spectral Line Data Reduction
Velocities in
Miriad
ATCA Spectral Line Correlator Configurations
Spectral Line Processing and RPFITS files
Spectral Line Processing and FITS files
Listing and Plotting Velocity Information
Recomputing Velocity Information
Setting the Rest Frequency
Velocity Linetype
Continuum Subtraction
Computation
Imaging and Image Velocity Definitions - INVERT and VELSW
Displaying Images
Introduction
The ATNF Visualisation Software
PGPLOT Device Tasks
Common Keywords
Examples
Image Analysis
Image Statistics and Histograms
Listing Image Values
Source Fitting and Positions
Copying, Reordering and Regridding Images
Image Arithmetic - MATHS
Smoothing Images
Modifying Images by Models
Polarimetric Analysis Tasks
Miscellaneous Analysis Tasks
Displaying Spectral Cubes
Introduction
The ATNF Visualisation Software
Displaying spectra only
Overlaying spectra on images
Analysing Spectral Cubes
Introduction
Moment Analysis
Smoothing the Velocity Axis
Velplot
Modelling galactic disks
Fitting a rotation curve
Fitting a tilted ring model to a warped galactic disk
Zeeman Analysis
Primary Beams and Mosaicing
Primary Beams and Primary Beam Correction
Mosaicing
Mosaicing Observing Strategies
Visibility Processing
Summary of Imaging Strategies
The Joint Approach
Imaging - INVERT
Deconvolution and Restoration
Self-Calibration
Some Additional Tools
The Individual Approach
Splitting and Imaging
Deconvolution, Restoration and Self-Calibration
Image Combination
Miscellaneous
Combining Mosaics and Single Dish Data
Some Theory and Preparing the Single-Dish Data
The Linear Method - IMMERGE
The Non-Linear Method - MOSMEM
Some Alternative Non-Linear Methods
Reducing 12-mm ATCA observations
Loading data into
Miriad
: ATLOD
Calibration
Reducing 3-mm ATCA observations
Some theory
Atmospheric opacity and system temperature
Antenna gain considerations and flux calibration
Instrumental phase
Atmospheric phase and phase calibration considerations
Flux density calibrators
Practical loading and calibration
Loading data into
Miriad
: ATLOD
Initial ``fixes'' to millimetre data
Additional monitoring variables
Reference pointing solutions
Seeing monitor measurement
Tracking accuracy
Bandpass and antenna gain calibration
Flux density bootstrapping
Information on planets
Handling large spectral bandwidths
ATCA Bin Mode Observations
ATCA Correlator Bin Modes
High time resolution bin-mode observations
Pulsar bin-mode observations
Tasks Specific to Pulsar Bin-Mode Observations
Setting Up Your Account
Image Items
UV Variables
Preparing Your Data in AIPS
Using xmtv and xpanel
Using xmtv
The Control Panel
Index
Miriad manager
2015-09-14