2019RAA....19...42L


Query : 2019RAA....19...42L

2019RAA....19...42L - Research in Astron. and astroph., 19, 42-42 (2019/March-0)

A deep learning approach for detecting candidates of supernova remnants.

LIU W., ZHU M., DAI C., WANG B.-Y., WU K., YU X.-C., TIAN W.-W., ZHANG M.-F. and WANG H.-F.

Abstract (from CDS):

Detecting supernova remnant (SNR) candidates in the interstellar medium is a challenging task because SNRs have weak radio signals and irregular shapes. The use of a convolutional neural network is a deep learning method that can help us extract various features from images. To extract SNRs from astronomical images and estimate the positions of SNR candidates, we design the SNR-Net model composed of a training component and a detection component. In addition, transfer learning is used to initialize the network parameters, which improves the speed and accuracy of network training. We apply a T-T plot (of the different brightness temperatures of map pixels at two different frequencies) to calculate the spectral index of SNR candidates. To accelerate the scientific computing process, we take advantage of innovative hardware architecture, such as deep learning optimized graphics processing units, which increases the speed of computation by a factor of 5. A case study suggests that SNR-Net may be applicable to detecting extended sources in the images automatically.

Abstract Copyright: ∼

Journal keyword(s): methods: data analysis - techniques: image processing - stars: fundamental parameters

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 NGC 6618 OpC 18 20 47 -16 10.3           ~ 1700 0
3 SNR G083.0-00.2 SNR 20 46.9 +42 52           ~ 21 0
4 SNR G084.2-00.8 SNR 20 53.3 +43 27           ~ 79 0
5 SNR G085.9-00.6 SNR 20 58.7 +44 53           ~ 32 0
6 NAME Local Group GrG ~ ~           ~ 9325 0

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