SYNCHROTRON TECHNOLOGY AND APPLICATIONSNo.1 1 Intermediate energy light sources and the SSRF project ZHAO Zhen—Tang9 Multiple scattering approach to X-ray absorption spectroscopyM.BENFATTO,Zi—Yu WU20 Electron gun fo...SYNCHROTRON TECHNOLOGY AND APPLICATIONSNo.1 1 Intermediate energy light sources and the SSRF project ZHAO Zhen—Tang9 Multiple scattering approach to X-ray absorption spectroscopyM.BENFATTO,Zi—Yu WU20 Electron gun for SSRFSHENG Shu—Gang,LIN Guo—Qiang,GU Qiang,LI De—Ming24 A new digital beam position monitor in SSRFCHENG Wei—Xing,LIU展开更多
For LAMOST, the largest sky survey program in China, the solution of the problem of automatic discrimination of stars from galaxies by spectra has shown that the results of the PSF test can be significantly refined. H...For LAMOST, the largest sky survey program in China, the solution of the problem of automatic discrimination of stars from galaxies by spectra has shown that the results of the PSF test can be significantly refined. However, the problem is made worse when the redshifts of galaxies are not available. We present a new automatic method of star/(normal) galaxy separation, which is based on Statistical Mixture Modeling with Radial Basis Function Neural Networks (SMM-RBFNN). This work is a continuation of our previous one, where active and non-active celestial objects were successfully segregated. By combining the method in this paper and the previous one, stars can now be effectively separated from galaxies and AGNs by their spectra-a major goal of LAMOST, and an indispensable step in any automatic spectrum classification system. In our work, the training set includes standard stellar spectra from Jacoby's spectrum library and simulated galaxy spectra of EO, SO, Sa, Sb types with redshift ranging from 0 to 1.2, and the test set of stellar spectra from Pickles' atlas and SDSS spectra of normal galaxies with SNR of 13. Experiments show that our SMM-RBFNN is more efficient in both the training and testing stages than the BPNN (back propagation neural networks), and more importantly, it can achieve a good classification accuracy of 99.22% and 96.52%, respectively for stars and normal galaxies.展开更多
An automated classification technique for large size stellar surveys is proposed. It uses the extended Kalman filter as a feature selector and pre-classifier of the data, and the radial basis function neural networks ...An automated classification technique for large size stellar surveys is proposed. It uses the extended Kalman filter as a feature selector and pre-classifier of the data, and the radial basis function neural networks for the classification. Experiments with real data have shown that the correct classification rate can reach as high as 93%, which is quite satisfactory. When different system models are selected for the extended Kalman filter, the classification results are relatively stable. It is shown that for this particular case the result using extended Kalman filter is better than using principal component analysis.展开更多
文摘SYNCHROTRON TECHNOLOGY AND APPLICATIONSNo.1 1 Intermediate energy light sources and the SSRF project ZHAO Zhen—Tang9 Multiple scattering approach to X-ray absorption spectroscopyM.BENFATTO,Zi—Yu WU20 Electron gun for SSRFSHENG Shu—Gang,LIN Guo—Qiang,GU Qiang,LI De—Ming24 A new digital beam position monitor in SSRFCHENG Wei—Xing,LIU
基金Supported by "863" National High Technology R&D program.
文摘For LAMOST, the largest sky survey program in China, the solution of the problem of automatic discrimination of stars from galaxies by spectra has shown that the results of the PSF test can be significantly refined. However, the problem is made worse when the redshifts of galaxies are not available. We present a new automatic method of star/(normal) galaxy separation, which is based on Statistical Mixture Modeling with Radial Basis Function Neural Networks (SMM-RBFNN). This work is a continuation of our previous one, where active and non-active celestial objects were successfully segregated. By combining the method in this paper and the previous one, stars can now be effectively separated from galaxies and AGNs by their spectra-a major goal of LAMOST, and an indispensable step in any automatic spectrum classification system. In our work, the training set includes standard stellar spectra from Jacoby's spectrum library and simulated galaxy spectra of EO, SO, Sa, Sb types with redshift ranging from 0 to 1.2, and the test set of stellar spectra from Pickles' atlas and SDSS spectra of normal galaxies with SNR of 13. Experiments show that our SMM-RBFNN is more efficient in both the training and testing stages than the BPNN (back propagation neural networks), and more importantly, it can achieve a good classification accuracy of 99.22% and 96.52%, respectively for stars and normal galaxies.
基金Supported by the National Natural Science Foundation of China (Project No. 60275002) The National High Technology Research and Development Program of China (863 Program, Project No.2003AA133060).
文摘An automated classification technique for large size stellar surveys is proposed. It uses the extended Kalman filter as a feature selector and pre-classifier of the data, and the radial basis function neural networks for the classification. Experiments with real data have shown that the correct classification rate can reach as high as 93%, which is quite satisfactory. When different system models are selected for the extended Kalman filter, the classification results are relatively stable. It is shown that for this particular case the result using extended Kalman filter is better than using principal component analysis.
