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Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.atnf.csiro.au/computing/software/miriad/userguide/
Дата изменения: Unknown
Дата индексирования: Sun Apr 10 12:30:54 2016
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Поисковые слова: sirds

userhtml

General Information
- Recommended Reading
- Acknowledgements
The User Interface
- Introduction
- The miriad Front-End
- 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
- 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
- Other Flagging Tasks
- Listing Visibilities
- Copying, Concatenating and Averaging Visibility Datasets
- Plotting Visibilities
- Examining Visibility Variables
- Modifying Visibility Datasets
Calibration, the ATCA, and Miriad
- Some Theory
- 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
- 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
- Deconvolution with maximum entropy algorithms
  - Computation
- Multi-frequency deconvolution - MFCLEAN
- Other deconvolution tasks
- Restoring an image
Self-Calibration
- Computation
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
- The Individual Approach
- Combining Mosaics and Single Dish Data
Reducing 12-mm ATCA observations
- Loading data into Miriad: ATLOD
- Calibration
Reducing 3-mm ATCA observations
- Some theory
- Practical loading and calibration
- 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