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