2024A&A...683A.104L


Query : 2024A&A...683A.104L

2024A&A...683A.104L - Astronomy and Astrophysics, volume 683A104 (2024/3-1)

Semi-supervised deep learning for molecular clump verification.

LUO X., ZHENG S., JIANG Z., CHEN Z., HUANG Y., ZENG S. and ZENG X.

Abstract (from CDS):

Context. A reliable molecular clump detection algorithm is essential for studying these clumps. Existing detection algorithms for molecular clumps still require that detected candidates be verified manually, which is impractical for large-scale data. Semi-supervised learning methods, especially those based on deep features, have the potential to accomplish the task of molecular clump verification thanks to the powerful feature extraction capability of deep networks.
Aims. Our main objective is to develop an automated method for the verification of molecular clump candidates. This method utilises a 3D convolutional neural network (3D CNN) to extract features of molecular clumps and employs semi-supervised learning to train the model, with the aim being to improve its generalisation ability and data utilisation. It addresses the issue of insufficient labelled samples in traditional supervised learning and enables the model to better adapt to new, unlabelled samples, achieving high accuracy in the verification of molecular clumps.
Methods. We propose SS-3D-Clump, a semi-supervised deep clustering method that jointly learns the parameters of a 3D CNN and the cluster assignments of the generated features for automatic verification of molecular clumps. SS-3D-Clump iteratively classifies the features with the Constrained-KMeans and uses these class labels as supervision to update the weights of the entire network.
Results. We used CO data from the Milky Way Imaging Scroll Painting project covering 350 square degrees in the Milky Way's first, second, and third quadrants. The ClumpFind algorithm was applied to extract molecular clump candidates in these regions, which were subsequently verified using SS-3D-Clump. The SS-3D-Clump model, trained on a dataset comprising three different density regions, achieved an accuracy of 0.933, a recall rate of 0.955, a precision rate of 0.945, and an F1 score of 0.950 on the corresponding test dataset. These results closely align with those obtained through manual verification.
Conclusions. Our experiments demonstrate that the SS-3D-Clump model achieves high accuracy in the automated verification of molecular clumps. It effectively captures the essential features of the molecular clumps and overcomes the challenge of limited labelled samples in supervised learning by using unlabelled samples through semi-supervised learning. This enhancement significantly improves the generalisation capability of the SS-3D-Clump model, allowing it to adapt effectively to new and unlabelled samples. Consequently, SS-3D-Clump can be integrated with any detection algorithm to create a comprehensive framework for the automated detection and verification of molecular clumps.

Abstract Copyright: © The Authors 2024

Journal keyword(s): dense matter - methods: data analysis - ISM: molecules

Simbad objects: 9

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Number of rows : 9
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ICRS (J2000)
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5 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
6 M 16 OpC 18 18 45.1 -13 47 31           ~ 1084 1
7 NAME Cyg X Cld 20 30 04.7973633 +40 51 36.002197           ~ 962 1
8 NAME Local Arm reg ~ ~           ~ 649 0
9 NAME Sct-Cen PoG ~ ~           ~ 286 0

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