Unresolved Galaxy Classifier for ESA/Gaia mission: Support Vector Machines approach

被引:0
|
作者
Bellas-Velidis, Ioannis [1 ]
Kontizas, Mary [2 ]
Dapergolas, Anastasios [1 ]
Livanou, Evdokia [2 ]
Kontizas, Evangelos [1 ]
Karampelas, Antonios [2 ]
机构
[1] Natl Observ Athens, Inst Astron & Astrophys, POB 20048, Athens 11810, Greece
[2] Univ Athens, Dept Astrophys Astron & Mech, Fac Phys, Athens 15783, Greece
来源
BULGARIAN ASTRONOMICAL JOURNAL | 2012年 / 18卷 / 02期
关键词
Methods: data analysis; Techniques: miscellaneous; Galaxies: general;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A software package Unresolved Galaxy Classifier (UGC) is being developed for the ground-based pipeline of ESA's Gaia mission. It aims to provide an automated taxonomic classification and specific parameters estimation analyzing Gaia BP/RP instrument low-dispersion spectra of unresolved galaxies. The UGC algorithm is based on a supervised learning technique, the Support Vector Machines (SVM). The software is implemented in Java as two separate modules. An offline learning module provides functions for SVM-models training. Once trained, the set of models can be repeatedly applied to unknown galaxy spectra by the pipeline's application module. A library of galaxy models synthetic spectra, simulated for the BP/RP instrument, is used to train and test the modules. Science tests show a very good classification performance of UGC and relatively good regression performance, except for some of the parameters. Possible approaches to improve the performance are discussed.
引用
收藏
页码:3 / 17
页数:15
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