---+++ Data selection: * -target=NAME Name of the astrophysical object * -effwave=LENGTH Effective wavelength, e.g. 1.6micron * -effband=LENGTH Effective bandwidth, e.g. 200nm * -wavemin=LENGTH Minimum wavelength, e.g. 1.5µm * -wavemax=LENGTH Maximum wavelength, e.g. 1.7µm ---+++ Which data to fit and how: * -use_vis=all|none|amp|phi Complex visibility data to consider * -use_vis2=all|none Powerspectrum data to consider * -use_t3=all|none|amp|phi Bispectrum data to consider * -convexcost=yes|no Use convex approximation for fitting complex data? * -phasecost=vonmises|haniff|convexlimit Co-log-likelihood approximation to use for phase data ---+++ Image parameters and direct model: * -pixelsize=ANGLE Angular size of pixels, e.g. 0.1mas * -fov=ANGLE Angular size of the field of view, e.g. 20mas * -imagesize=DIM|DIM1xDIM2 Number of pixels per side of the image * -flux=VALUE Total flux (sum of pixels = VALUE) * -fluxerr=VALUE Assumed standard deviation for the total flux * -min=LOWER Lower bound for the pixel values * -max=UPPER Upper bound for the pixel values * -xform=nfft|separable|nonseparable Method to compute the Fourier transform * -smearingfunction=none|sinc|gauss Method to model the effects of the spectral bandwidth smearing * -smearingfactor=VALUE Factor to scale the effects of the spectral bandwidth smearing * -nthreads=NUMBER Number of threads for the fast Fourier transform ---+++ Regularization settings: * -regul=NAME Name of regularization method (-regul=help for more information) * -mu=VALUE(S) Global regularization weight ---++++ Available regularizations: * -regul=hyperbolic -tau=... Edge-preserving smoothness with hyperbolic norm, approximates total variation (TV) with TAU very small. * -tau=VALUE Edge preserving threshold * -eta=VALUE(S) Gradient scales along dimensions * -regul=compactness -gamma=... Quadratic compactness with full-width at half maximum GAMMA. * -gamma=FWHM A priori full half width at half maximum, e.g. 15mas ---+++ Initial image: * -initial=NAME FITS file or method for initial image * -seed=VALUE Seed for the random generator ---+++ Output file: * -save_visibilities Save model complex visibilities * -overwrite Overwrite output if it exists * -bitpix=BITPIX Bits per pixel * -save_initial Save initial image as a secondary HDU in the result ---+++ Reconstruction strategy: * -bootstrap=COUNT Number of bootstrapping iterations * -recenter Recenter result of bootstrapping iterations * -threshold=FRACTION Level for soft-thresholding input image(s) ---+++ Messages: * -quiet Suppress most messages * -verb=COUNT Verbose level ---+++ Optimizer Settings: * -mem=COUNT Number of previous steps to memorize in VMLMB * -ftol=REAL Function tolerance for the global convergence * -gtol=REAL Gradient tolerance for the global convergence * -maxiter=COUNT Maximum number of iterations * -maxeval=COUNT Maximum number of evaluations of the objective function ---+++ Line search: * -sftol=REAL Function tolerance for the line search * -sgtol=REAL Gradient tolerance for the line search * -sxtol=REAL Step tolerance for the line search ---+++ Miscellaneous: * -settings=NAME Name of the FITS parameter file * -plugin=NAME Name of plugin * -debug Debug mode * -help Print out this help * -version Print out version number
This topic: Jmmc/Software
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Topic revision: r1 - 2018-09-21 - FerreolSoulez
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