Hybrid Very Long Baseline Interferometry Imaging and Modeling withthemis

被引:46
作者
Broderick, Avery E. [1 ,2 ,3 ]
Pesce, Dominic W. [4 ,5 ]
Tiede, Paul [1 ,2 ,3 ]
Pu, Hung-Yi [1 ]
Gold, Roman [1 ,6 ,7 ]
机构
[1] Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
[2] Univ Waterloo, Dept Phys & Astron, 200 Univ Ave West, Waterloo, ON N2L 3G1, Canada
[3] Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada
[4] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA
[5] Harvard Univ, Black Hole Initiat, 20 Garden St, Cambridge, MA 02138 USA
[6] Univ Southern Denmark, Origins CP3, Campusvej 55, DK-5230 Odense M, Denmark
[7] Goethe Univ Frankfurt, Inst Theoret Phys, Max von Laue Str 1, D-60438 Frankfurt, Germany
基金
加拿大创新基金会; 加拿大自然科学与工程研究理事会;
关键词
Black Hole physics; Astronomy data modeling; Computational astronomy; Submillimeter astronomy; Long baseline interferometry; General relativity; SELF-CALIBRATION; RADIO; RECONSTRUCTION;
D O I
10.3847/1538-4357/ab9c1f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Generating images from very long baseline interferometric observations poses a difficult, and generally not unique, inversion problem. This problem is simplified by the introduction of constraints, some generic (e.g., positivity of the intensity) and others motivated by physical considerations (e.g., smoothness, instrument resolution). It is further complicated by the need to simultaneously address instrumental systematic uncertainties and sparse coverage in theu-vplane. We report a new Bayesian image reconstruction technique in the parameter estimation framework Themisthat has been developed for the Event Horizon Telescope. This has two key features: first, the full Bayesian treatment of the image reconstruction makes it possible to generate a full posterior for the images, permitting a rigorous and quantitative investigation into the statistical significance of image features. Second, it is possible to seamlessly incorporate directly modeled features simultaneously with image reconstruction. We demonstrate this second capability by incorporating a narrow, slashed ring in reconstructions of simulated M87 data in an attempt to detect and characterize the photon ring. We show that it is possible to obtain high-fidelity photon ring sizes, enabling mass measurements with accuracies of 2%-5% that are essentially insensitive to astrophysical uncertainties, and creating opportunities for precision tests of general relativity.
引用
收藏
页数:15
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