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MIRA(1) General Commands Manual MIRA(1)

NAME

MiRA - a Multi-aperture Image Reconstruction Algorithm

SYNOPSIS

mira [OPTIONS] INPUT [...] OUTPUT

DESCRIPTION

MiRA - a Multi-aperture Image Reconstruction Algorithm INPUT and [...] are the OI-FITS data file and OUTPUT is the result saved into a FITS file.

Name of the astrophysical object
Effective wavelength, e.g. 1.6micron
Effective bandwidth, e.g. 200nm
Minimum wavelength, e.g. 1.5??m
Maximum wavelength, e.g. 1.7??m
Angular size of pixels, e.g. 0.1mas
Angular size of the field of view, e.g. 20mas
Number of pixels per side of the image
Method to compute the Fourier transform
Flux normalization (sum of pixels = VALUE)
Lower bound for the pixel values
Upper bound for the pixel values
Overwrite output if it exists
Name of regularization method
Global regularization weight
Edge preserving threshold
Gradient scales along dimensions
A priori full half width at half maximum, e.g. 15mas
FITS file or method for initial image
Seed for the random generator
Save initial image as a secondary HDU in result
Number of bootstrapping iterations
Recenter result of bootstrapping iterations
Level for soft-thresholding input image(s)
Maximum number of iterations
Maximum number of evaluations of the objective function
Suppress most messages
Verbose level
Bitwise mask to specify which graphics to show
Number of previous steps to memorize in VMLMB
Function tolerance for the global convergence
Gradient tolerance for the global convergence
Function tolerance for the line search
Gradient tolerance for the line search
Step tolerance for the line search
Bits per pixel
Print out this help
Print out version number
Science User Commands