PRECL: A new method for interferometry imaging from closure phase
暂无分享,去创建一个
Kazunori Akiyama | Fumie Tazaki | Shiro Ikeda | Mareki Honma | Kazuhiro Hada | S. Ikeda | K. Akiyama | M. Honma | F. Tazaki | K. Hada | Shiro Ikeda
[1] Alan E. E. Rogers,et al. PERSISTENT ASYMMETRIC STRUCTURE OF SAGITTARIUS A* ON EVENT HORIZON SCALES , 2016, 1602.05527.
[2] Alan E. E. Rogers,et al. 230 GHz VLBI OBSERVATIONS OF M87: EVENT‐HORIZON‐SCALE STRUCTURE DURING AN ENHANCED VERY‐HIGH‐ENERGY γ ?> ‐RAY STATE IN 2012 , 2015, 1505.03545.
[3] Kazunori Akiyama,et al. Super-resolution imaging with radio interferometry using sparse modeling , 2014, 1407.2422.
[4] M. Kino,et al. A STRONG RADIO BRIGHTENING AT THE JET BASE OF M 87 DURING THE ELEVATED VERY HIGH ENERGY GAMMA-RAY STATE IN 2012 , 2014, 1405.1082.
[5] Canada.,et al. IMAGING THE SUPERMASSIVE BLACK HOLE SHADOW AND JET BASE OF M87 WITH THE EVENT HORIZON TELESCOPE , 2014, 1404.7095.
[6] Mareki Honma,et al. High-Angular-Resolution and High-Sensitivity Science Enabled by Beamformed ALMA , 2013, 1309.3519.
[7] Mareki Honma,et al. THE INNERMOST COLLIMATION STRUCTURE OF THE M87 JET DOWN TO ∼10 SCHWARZSCHILD RADII , 2013, 1308.1411.
[8] M. Wright,et al. FINE-SCALE STRUCTURE OF THE QUASAR 3C 279 MEASURED WITH 1.3 mm VERY LONG BASELINE INTERFEROMETRY , 2013, 1305.3359.
[9] Alan E. E. Rogers,et al. Jet-Launching Structure Resolved Near the Supermassive Black Hole in M87 , 2012, Science.
[10] M. Kino,et al. VLBI OBSERVATIONS OF THE JET IN M 87 DURING THE VERY HIGH ENERGY γ-RAY FLARE IN 2010 APRIL , 2012, 1210.4942.
[11] RESOLVING THE INNER JET STRUCTURE OF 1924-292 WITH THE EVENT HORIZON TELESCOPE , 2012, 1208.4402.
[12] Eric Agol,et al. The size of the jet launching region in M87 , 2011, 1109.6011.
[13] Noriyuki Kawaguchi,et al. An origin of the radio jet in M87 at the location of the central black hole , 2011, Nature.
[14] M. Wright,et al. 1.3 mm WAVELENGTH VLBI OF SAGITTARIUS A*: DETECTION OF TIME-VARIABLE EMISSION ON EVENT HORIZON SCALES , 2010, 1011.2472.
[15] Marc Teboulle,et al. Fast Gradient-Based Algorithms for Constrained Total Variation Image Denoising and Deblurring Problems , 2009, IEEE Transactions on Image Processing.
[16] A. Loeb,et al. IMAGING THE BLACK HOLE SILHOUETTE OF M87: IMPLICATIONS FOR JET FORMATION AND BLACK HOLE SPIN , 2008, 0812.0366.
[17] Marc Teboulle,et al. A Fast Iterative Shrinkage-Thresholding Algorithm for Linear Inverse Problems , 2009, SIAM J. Imaging Sci..
[18] Canadian Institute for Theoretical Astrophysics,et al. DETECTING FLARING STRUCTURES IN SAGITTARIUS A* WITH HIGH-FREQUENCY VLBI , 2008, 0809.3424.
[19] A. Niell,et al. Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre , 2008, Nature.
[20] M. Bershady,et al. SparsePak: A Formatted Fiber Field Unit for the WIYN Telescope Bench Spectrograph. I. Design, Construction, and Calibration , 2004, astro-ph/0403456.
[21] N. Kawaguchi,et al. An Imaging Algorithm Using the Bispectrum in Radio Interferometry , 1997 .
[22] Alan E. E. Rogers,et al. Fringe Detection Methods for Very Long Baseline Arrays , 1995 .
[23] W. J. Tango,et al. Very High Angular Resolution Imaging , 1994 .
[24] T. Cornwell,et al. A new method for making maps with unstable radio interferometers , 1981 .
[25] Alan E. E. Rogers,et al. The structure of radio sources 3C 273B and 3C 84 deduced from the "closure" phases and visibility amplitudes observed with three-element interferometers. , 1974 .
[26] R. Jennison. A Phase Sensitive Interferometer Technique for the Measurement of the Fourier Transforms of Spatial Brightness Distributions of Small Angular Extent , 1958 .