4.7 Article

Scalable precision wide-field imaging in radio interferometry - II. AIRI validated on ASKAP data

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 522, Issue 4, Pages 5576-5587

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stad1353

Keywords

techniques: image processing; techniques: interferometric; galaxies: clusters: intracluster medium; radio continuum: galaxies

Ask authors/readers for more resources

This paper validates the recently proposed AIRI algorithm on observations from ASKAP, showcasing monochromatic AIRI-ASKAP images formed using a parallelized and automated imaging framework. AIRI differs from uSARA by using a trained DNN for the regularization step in deconvolution and evaluates the reconstruction variations. The scientific potential delivered by AIRI is evident in improved reconstruction of diffuse components, accurate spectral index maps, and significant acceleration in deconvolution time.
Accompanying Part I, this sequel delineates a validation of the recently proposed AI for Regularization in radio-interferometric Imaging (AIRI) algorithm on observations from the Australian Square Kilometre Array Pathfinder (ASKAP). The monochromatic AIRI-ASKAP images showcased in this work are formed using the same parallelized and automated imaging framework described in Part I: 'uSARA validated on ASKAP data'. Using a Plug-and-Play approach, AIRI differs from uSARA by substituting a trained denoising deep neural network (DNN) for the proximal operator in the regularization step of the forward-backward algorithm during deconvolution. We build a trained shelf of DNN denoisers that target the estimated image dynamic ranges of our selected data. Furthermore, we quantify variations of AIRI reconstructions when selecting the nearest DNN on the shelf versus using a universal DNN with the highest dynamic range, opening the door to a more complete framework that not only delivers image estimation but also quantifies epistemic model uncertainty. We continue our comparative analysis of source structure, diffuse flux measurements, and spectral index maps of selected target sources as imaged by AIRI and the algorithms in Part I - uSARA and WSClean. Overall, we see an improvement over uSARA and WSClean in the reconstruction of diffuse components in AIRI images. The scientific potential delivered by AIRI is evident in further imaging precision, more accurate spectral index maps, and a significant acceleration in deconvolution time, whereby AIRI is four times faster than its subiterative sparsity-based counterpart uSARA.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available