“…U-Net++ [49] proposes a combination of architectural improvements by improving the skip connection pathways and extending the deep supervision mechanism, while Tiramisu [50] employs DenseNets [51] instead of ResNets [34] improving the performance using fewer parameters. Other approaches [11,52] propose hierarchical decoding for segmentation, which, instead of employing the pipeline of downsampling and upsampling path, decode features at multiple resolutions and combine them at the end.…”
Section: Related Workmentioning
confidence: 99%
“…Then the image is expanded back to the original image size in the decoding path to obtain the binary masks that classify the objects. There are many variants that extend this framework by applying skip connections [47], deep supervision [48], or hierarchical decoding [11].…”
Section: Architecturesmentioning
confidence: 99%
“…In our analysis, we employ the following architectures on our radio-astronomical dataset, as shown in Fig. 5: a basic encoder-decoder architecture, U-Net [47], which adds skip connections to the basic architecture, U-Net with deep supervision, which enhances the loss by computing it also on intermediate upsampled masks, Tiramisu [50], which employs DenseNets [51] instead of convolutions in the downsampling and upsampling blocks, and PankNet [11], which makes use of hierarchical decoding for information mixing between upsampling paths.…”
Section: Segmentation Modelsmentioning
confidence: 99%
“…Finally, we employ PankNet [11], which does not make use of the downsampling-upsampling pipeline but applies encoders and decoders in a multilevel way, as shown in Fig 5(d). Each decoder receives only the corresponding encoder output as input, while the other versions concatenated it to the previous decoder output.…”
Section: Panknetmentioning
confidence: 99%
“…To overcome these limitations, deep learning models represent the evolution of such approaches and yield interesting results extensively explored in several domains. In particular, object detection and semantic segmentation models based on deep learning are currently used in different domains, such as automotive [5][6][7][8], medical imaging [9][10][11], video surveillance [12,13], and robot navigation [14][15][16]. The radio-astronomical domain has not yet been exhaustively explored with the application of the mentioned methods; therefore, this work represents an attempt to gather performance and computational requirements about several state-of-the-art approaches to be used as a reference for future work.…”
In recent years, deep learning has been successfully applied in various scientific domains. Following these promising results and performances, it has recently also started being evaluated in the domain of radio astronomy. In particular, since radio astronomy is entering the Big Data era, with the advent of the largest telescope in the world -the Square Kilometre Array (SKA), the task of automatic object detection and instance segmentation is crucial for source finding and analysis. In this work, we explore the performance of the most affirmed deep learning approaches, applied to astronomical images obtained by radio interferometric instrumentation, to solve the task of automatic source detection. This is carried out by applying models designed to accomplish two different kinds of tasks: object detection and semantic segmentation. The goal is
“…U-Net++ [49] proposes a combination of architectural improvements by improving the skip connection pathways and extending the deep supervision mechanism, while Tiramisu [50] employs DenseNets [51] instead of ResNets [34] improving the performance using fewer parameters. Other approaches [11,52] propose hierarchical decoding for segmentation, which, instead of employing the pipeline of downsampling and upsampling path, decode features at multiple resolutions and combine them at the end.…”
Section: Related Workmentioning
confidence: 99%
“…Then the image is expanded back to the original image size in the decoding path to obtain the binary masks that classify the objects. There are many variants that extend this framework by applying skip connections [47], deep supervision [48], or hierarchical decoding [11].…”
Section: Architecturesmentioning
confidence: 99%
“…In our analysis, we employ the following architectures on our radio-astronomical dataset, as shown in Fig. 5: a basic encoder-decoder architecture, U-Net [47], which adds skip connections to the basic architecture, U-Net with deep supervision, which enhances the loss by computing it also on intermediate upsampled masks, Tiramisu [50], which employs DenseNets [51] instead of convolutions in the downsampling and upsampling blocks, and PankNet [11], which makes use of hierarchical decoding for information mixing between upsampling paths.…”
Section: Segmentation Modelsmentioning
confidence: 99%
“…Finally, we employ PankNet [11], which does not make use of the downsampling-upsampling pipeline but applies encoders and decoders in a multilevel way, as shown in Fig 5(d). Each decoder receives only the corresponding encoder output as input, while the other versions concatenated it to the previous decoder output.…”
Section: Panknetmentioning
confidence: 99%
“…To overcome these limitations, deep learning models represent the evolution of such approaches and yield interesting results extensively explored in several domains. In particular, object detection and semantic segmentation models based on deep learning are currently used in different domains, such as automotive [5][6][7][8], medical imaging [9][10][11], video surveillance [12,13], and robot navigation [14][15][16]. The radio-astronomical domain has not yet been exhaustively explored with the application of the mentioned methods; therefore, this work represents an attempt to gather performance and computational requirements about several state-of-the-art approaches to be used as a reference for future work.…”
In recent years, deep learning has been successfully applied in various scientific domains. Following these promising results and performances, it has recently also started being evaluated in the domain of radio astronomy. In particular, since radio astronomy is entering the Big Data era, with the advent of the largest telescope in the world -the Square Kilometre Array (SKA), the task of automatic object detection and instance segmentation is crucial for source finding and analysis. In this work, we explore the performance of the most affirmed deep learning approaches, applied to astronomical images obtained by radio interferometric instrumentation, to solve the task of automatic source detection. This is carried out by applying models designed to accomplish two different kinds of tasks: object detection and semantic segmentation. The goal is
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