New Frontiers in Stellar Interferometry 2004
DOI: 10.1117/12.550710
|View full text |Cite
|
Sign up to set email alerts
|

An interferometry imaging beauty contest

Abstract: We present a formal comparison of the performance of algorithms used for synthesis imaging with optical/infrared long-baseline interferometers. Five different algorithms are evaluated based on their performance with simulated test data. Each set of test data is formatted in the OI-FITS format. The data are calibrated power spectra and bispectra measured with an array intended to be typical of existing imaging interferometers. The strengths and limitations of each algorithm are discussed.

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
38
0

Year Published

2008
2008
2018
2018

Publication Types

Select...
6
2
1

Relationship

1
8

Authors

Journals

citations
Cited by 52 publications
(38 citation statements)
references
References 12 publications
0
38
0
Order By: Relevance
“…Figure 4 shows an image of LkHα 101 observed at wavelength of 550 nm, which covers 12 milli-arcsecond (mas) along both axes. The LkHα 101 has the diameter of about 5.5 mas [17], and is located at the right ascension of 4 h 30 m 14.4 s , the declination of 35 • 16 24 , and at a distance of 700 parsec (pc) from the Earth [17]. This image will be used as the reference imagex ref for simulations, which is composed of 256 × 256 pixels, with an angular resolution of 0.0469 mas/pixel.…”
Section: Optimal Solutionmentioning
confidence: 99%
See 1 more Smart Citation
“…Figure 4 shows an image of LkHα 101 observed at wavelength of 550 nm, which covers 12 milli-arcsecond (mas) along both axes. The LkHα 101 has the diameter of about 5.5 mas [17], and is located at the right ascension of 4 h 30 m 14.4 s , the declination of 35 • 16 24 , and at a distance of 700 parsec (pc) from the Earth [17]. This image will be used as the reference imagex ref for simulations, which is composed of 256 × 256 pixels, with an angular resolution of 0.0469 mas/pixel.…”
Section: Optimal Solutionmentioning
confidence: 99%
“…An image of LkHα 101 [17] is adopted for testing in this work, and the optical interferometric data are simulated on the configuration of the six-station Navy Prototype Optical Interferometer (NPOI) [18] plus GRAVITY to verify the efficacy of the proposed method. If the brightness distribution has a weak dependence on wavelengths [9,19], polychromatic measurement data can be used to further enhance the reconstructed image [14,20].…”
Section: Introductionmentioning
confidence: 99%
“…The original cube with a pixel resolution of 0.1 mas is of size 501 × 501 pixels ×30 channels, the field of view (FOV) is ≈ 50 mas. The instrumental configuration was used in the 2004 International Beauty Contest in Optical Interferometry [51]: Thirty equi-spaced wavelengths in the range 1.45 µm − 1.84 µm (high resolution) at 13 acquisition instants are analyzed. The spatial frequencies coverage, including the earth rotation effect, is shown in Fig.…”
Section: Resolved Stars Reconstructionmentioning
confidence: 99%
“…Examples include the BBM method (building block mapping; Hofmann & Weigelt 1993;Hofmann et al 2005), BSMEM (bispectrum maximum entropy method; Buscher 1994), MIRA (multi-aperture image reconstruction algorithm; Thiebaut 2002), and MACIM (Monte-Carlo imaging; Ireland et al 2006). The performance of various algorithms was evaluated in several blind tests (Lawson et al 2004(Lawson et al , 2006Malbet et al 2010;Baron et al 2012) initiated by the IAU Working Group on Optical/IR Interferometry. In contrast to our BBM method, the new IRBis method (image reconstruction software using the bispectrum) employs a fast minimization routine based on conjugate gradients (Hager & Zhang 2005.…”
Section: Introductionmentioning
confidence: 99%