Super-resolution imaging with radio interferometry using sparse modeling

We propose a new technique to obtain super-resolution images with radio interferometer using sparse modeling. In standard radio interferometry, sampling of ($u$, $v$) is quite often incomplete and thus obtaining an image from observed visibilities becomes an underdetermined problem, and a technique so-called "zero-padding" is often used to fill up unsampled grids in ($u$, $v$) plane, resulting in image degradation by finite beam size as well as numerous side-lobes. In this paper we show that directly solving such an underdetermined problem based on sparse modeling (in this paper LASSO) avoids the above problems introduced by zero-padding, leading to super-resolution images in which structure finer than the standard beam size (diffraction limit) can be reproduced. We present results of one-dimensional and two-dimensional simulations of interferometric imaging, and discuss its implications to super-resolution imaging, particularly focusing on imaging of black hole shadows with millimeter VLBI.

[1]  A. Niell,et al.  Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre , 2008, Nature.

[2]  Feng Li,et al.  The application of compressive sampling to radio astronomy I: Deconvolution , 2011, 1106.1711.

[3]  M. Wright,et al.  FINE-SCALE STRUCTURE OF THE QUASAR 3C 279 MEASURED WITH 1.3 mm VERY LONG BASELINE INTERFEROMETRY , 2013, 1305.3359.

[4]  Taichi Kato,et al.  Period Analysis using the Least Absolute Shrinkage and Selection Operator (Lasso) , 2012, 1205.4791.

[5]  Alan E. E. Rogers,et al.  Jet-Launching Structure Resolved Near the Supermassive Black Hole in M87 , 2012, Science.

[6]  I. Daubechies,et al.  An iterative thresholding algorithm for linear inverse problems with a sparsity constraint , 2003, math/0307152.

[7]  Marcus Magnor,et al.  SparseRI: A Compressed Sensing Framework for Aperture Synthesis Imaging in Radio Astronomy , 2010 .

[8]  M. Lustig,et al.  Compressed Sensing MRI , 2008, IEEE Signal Processing Magazine.

[9]  Canadian Institute for Theoretical Astrophysics,et al.  DETECTING FLARING STRUCTURES IN SAGITTARIUS A* WITH HIGH-FREQUENCY VLBI , 2008, 0809.3424.

[10]  RESOLVING THE INNER JET STRUCTURE OF 1924-292 WITH THE EVENT HORIZON TELESCOPE , 2012, 1208.4402.

[11]  J. A. Zensus,et al.  “RadioAstron”-A telescope with a size of 300 000 km: Main parameters and first observational results , 2013, 1303.5013.

[12]  Shibata,et al.  Overview and initial results of the very long baseline interferometry space observatory programme , 1998, Science.

[13]  Karl Gebhardt,et al.  THE BLACK HOLE MASS, STELLAR MASS-TO-LIGHT RATIO, AND DARK HALO IN M87 , 2009, 0906.1492.

[14]  David F. Buscher Direct Maximum-Entropy Image Reconstruction from the Bispectrum , 1994 .

[15]  Emmanuel J. Candès,et al.  Near-Optimal Signal Recovery From Random Projections: Universal Encoding Strategies? , 2004, IEEE Transactions on Information Theory.

[16]  P. Vandergheynst,et al.  Compressed sensing imaging techniques for radio interferometry , 2008, 0812.4933.

[17]  Alan E. E. Rogers,et al.  Fringe Detection Methods for Very Long Baseline Arrays , 1995 .

[18]  University of California,et al.  THE M87 BLACK HOLE MASS FROM GAS-DYNAMICAL MODELS OF SPACE TELESCOPE IMAGING SPECTROGRAPH OBSERVATIONS , 2013, 1304.7273.

[19]  A. Marconi,et al.  The Supermassive Black Hole of M87 and the Kinematics of Its Associated Gaseous Disk , 1997 .

[20]  Shiro Ikeda,et al.  Phase retrieval from single biomolecule diffraction pattern. , 2011, Optics express.