Astrophysics > Instrumentation and Methods for Astrophysics
            [Submitted on 2 Mar 2014
            
            
            
            ]
          
          Title: Automatic classification of time-variable X-ray sources
Title: 时变X射线源的自动分类
Abstract: To maximize the discovery potential of future synoptic surveys, especially in the field of transient science, it will be necessary to use automatic classification to identify some of the astronomical sources. The data mining technique of supervised classification is suitable for this problem. Here, we present a supervised learning method to automatically classify variable X-ray sources in the second \textit{XMM-Newton} serendipitous source catalog (2XMMi-DR2). Random Forest is our classifier of choice since it is one of the most accurate learning algorithms available. Our training set consists of 873 variable sources and their features are derived from time series, spectra, and other multi-wavelength contextual information. The 10-fold cross validation accuracy of the training data is ${\sim}$97% on a seven-class data set. We applied the trained classification model to 411 unknown variable 2XMM sources to produce a probabilistically classified catalog. Using the classification margin and the Random Forest derived outlier measure, we identified 12 anomalous sources, of which, 2XMM J180658.7$-$500250 appears to be the most unusual source in the sample. Its X-ray spectra is suggestive of a ULX but its variability makes it highly unusual. Machine-learned classification and anomaly detection will facilitate scientific discoveries in the era of all-sky surveys.
          Current browse context: 
        
          astro-ph.IM
          
          
          
          
          
          
            
            
              Change to browse by:
              
            
            
          
        References & Citations
Bibliographic and Citation Tools
            Bibliographic Explorer (What is the Explorer?)
          
        
            Connected Papers (What is Connected Papers?)
          
        
            Litmaps (What is Litmaps?)
          
        
            scite Smart Citations (What are Smart Citations?)
          
        Code, Data and Media Associated with this Article
            alphaXiv (What is alphaXiv?)
          
        
            CatalyzeX Code Finder for Papers (What is CatalyzeX?)
          
        
            DagsHub (What is DagsHub?)
          
        
            Gotit.pub (What is GotitPub?)
          
        
            Hugging Face (What is Huggingface?)
          
        
            Papers with Code (What is Papers with Code?)
          
        
            ScienceCast (What is ScienceCast?)
          
        Demos
Recommenders and Search Tools
              Influence Flower (What are Influence Flowers?)
            
          
              CORE Recommender (What is CORE?)
            
          
              IArxiv Recommender
              (What is IArxiv?)
            
          arXivLabs: experimental projects with community collaborators
arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.
Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.
Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.
 
  