Deep Learning for Spectrum Prediction from Spatial-Temporal-Spectral Data

2020 ◽  
pp. 1-1
Author(s):  
Xi Li ◽  
Zhicheng Liu ◽  
Guojun Chen ◽  
Yinfei Xu ◽  
Tiecheng Song
2020 ◽  
Author(s):  
Ching Tarn ◽  
Wen-Feng Zeng ◽  
Zhengcong Fei ◽  
Si-Min He

AbstractSpectrum prediction using deep learning has attracted a lot of attention in recent years. Although existing deep learning methods have dramatically increased the prediction accuracy, there is still considerable space for improvement, which is presently limited by the difference of fragmentation types or instrument settings. In this work, we use the few-shot learning method to fit the data online to make up for the shortcoming. The method is evaluated using ten datasets, where the instruments includes Velos, QE, Lumos, and Sciex, with collision energies being differently set. Experimental results show that few-shot learning can achieve higher prediction accuracy with almost negligible computing resources. For example, on the dataset from a untrained instrument Sciex-6600, within about 10 seconds, the prediction accuracy is increased from 69.7% to 86.4%; on the CID (collision-induced dissociation) dataset, the prediction accuracy of the model trained by HCD (higher energy collision dissociation) spectra is increased from 48.0% to 83.9%. It is also shown that, the method is not critical to data quality and is sufficiently efficient to fill the accuracy gap. The source code of pDeep3 is available at http://pfind.ict.ac.cn/software/pdeep3.


2020 ◽  
Vol 103 (10) ◽  
pp. 9355-9367
Author(s):  
S.J. Denholm ◽  
W. Brand ◽  
A.P. Mitchell ◽  
A.T. Wells ◽  
T. Krzyzelewski ◽  
...  

Author(s):  
Jun Zhou ◽  
Zheng Zhu ◽  
Jiajia Qian ◽  
Zhenzhen Ge ◽  
Shuting Wu

IEEE Access ◽  
2019 ◽  
Vol 7 ◽  
pp. 45818-45830 ◽  
Author(s):  
Ruben Mennes ◽  
Maxim Claeys ◽  
Felipe A. P. De Figueiredo ◽  
Irfan Jabandzic ◽  
Ingrid Moerman ◽  
...  

2020 ◽  
Vol 2020 (1) ◽  
pp. 134-138
Author(s):  
Tarek Stiebel ◽  
Dorit Merhof

Spectral recovery from measured camera signals based on deep learning lead to significant advancements of the potential reconstruction quality. However, most deep learning based approaches only consider RGB cameras and are targeting object classification in particular or remote sensing in general as their final application. Within this work, we analyze the influence of a joint filter optimization and spectral recovery for multi-spectral image acquisition with the underlying goal of capturing high-fidelity color images. An evaluation on the influence of the total camera channel count on the reproduction quality is provided. Finally, a possible normalization of spectral data is discussed.


2017 ◽  
Author(s):  
King Ma ◽  
Henry Leung ◽  
Ehsan Jalilian ◽  
Daniel Huang

2019 ◽  
Vol 488 (3) ◽  
pp. 4106-4116 ◽  
Author(s):  
Hiroyoshi Iwasaki ◽  
Yuto Ichinohe ◽  
Yasunobu Uchiyama

ABSTRACT Recent rapid development of deep learning algorithms, which can implicitly capture structures in high-dimensional data, opens a new chapter in astronomical data analysis. We report here a new implementation of deep learning techniques for X-ray analysis. We apply a variational autoencoder (VAE) using a deep neural network for spatio-spectral analysis of data obtained by Chandra X-ray Observatory from Tycho’s supernova remnant (SNR). We established an unsupervised learning method combining the VAE and a Gaussian mixture model (GMM), where the dimensions of the observed spectral data are reduced by the VAE, and clustering in feature space is performed by the GMM. We found that some characteristic spatial structures, such as the iron knot on the eastern rim, can be automatically recognized by this method, which uses only spectral properties. This result shows that unsupervised machine learning can be useful for extracting characteristic spatial structures from spectral information in observational data (without detailed spectral analysis), which would reduce human-intensive preprocessing costs for understanding fine structures in diffuse astronomical objects, e.g. SNRs or galaxy clusters. Such data-driven analysis can be used to select regions from which to extract spectra for detailed analysis and help us make the best use of the large amount of spectral data available currently and arriving in the coming decades.


Sign in / Sign up

Export Citation Format

Share Document