TY - JOUR
T1 - DECORAS
T2 - Detection and characterization of radio-astronomical sources using deep learning
AU - Rezaei, S.
AU - McKean, J. P.
AU - Biehl, M.
AU - Javadpour, A.
N1 - Publisher Copyright:
© The Author(s) 2021.
PY - 2022/3/1
Y1 - 2022/3/1
N2 - We present DECORAS, a deep-learning-based approach to detect both point and extended sources from Very Long Baseline Interferometry (VLBI) observations. Our approach is based on an encoder-decoder neural network architecture that uses a low number of convolutional layers to provide a scalable solution for source detection. In addition, DECORAS performs source characterization in terms of the position, effective radius, and peak brightness of the detected sources. We have trained and tested the network with images that are based on realistic Very Long Baseline Array (VLBA) observations at 20 cm. Also, these images have not gone through any prior de-convolution step and are directly related to the visibility data via a Fourier transform. We find that the source catalogue generated by DECORAS has a better overall completeness and purity, when compared to a traditional source detection algorithm. DECORAS is complete at the 7.5σ level, and has an almost factor of 2 improvement in purity at 5.5σ. We find that DECORAS can recover the position of the detected sources to within 0.61 ± 0.69 mas, and the effective radius and peak surface brightness are recovered to within 20 per cent for 98 and 94 per cent of the sources, respectively. Overall, we find that DECORAS provides a reliable source detection and characterization solution for future wide-field VLBI surveys.
AB - We present DECORAS, a deep-learning-based approach to detect both point and extended sources from Very Long Baseline Interferometry (VLBI) observations. Our approach is based on an encoder-decoder neural network architecture that uses a low number of convolutional layers to provide a scalable solution for source detection. In addition, DECORAS performs source characterization in terms of the position, effective radius, and peak brightness of the detected sources. We have trained and tested the network with images that are based on realistic Very Long Baseline Array (VLBA) observations at 20 cm. Also, these images have not gone through any prior de-convolution step and are directly related to the visibility data via a Fourier transform. We find that the source catalogue generated by DECORAS has a better overall completeness and purity, when compared to a traditional source detection algorithm. DECORAS is complete at the 7.5σ level, and has an almost factor of 2 improvement in purity at 5.5σ. We find that DECORAS can recover the position of the detected sources to within 0.61 ± 0.69 mas, and the effective radius and peak surface brightness are recovered to within 20 per cent for 98 and 94 per cent of the sources, respectively. Overall, we find that DECORAS provides a reliable source detection and characterization solution for future wide-field VLBI surveys.
KW - Methods: Data analysis
KW - Radio continuum: Galaxies
KW - Techniques: Image processing
KW - Techniques: Interferometric
UR - http://www.scopus.com/inward/record.url?scp=85125126157&partnerID=8YFLogxK
U2 - 10.1093/mnras/stab3519
DO - 10.1093/mnras/stab3519
M3 - Article
SN - 0035-8711
VL - 510
SP - 5891
EP - 5907
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 4
ER -