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                    Evans, P.A., Beardmore, A.P., Page, K.L., Tyler, L.G., Osborne, J.P., Goad, M.R., et al. (2007) An Online Repository of Swift/XRT Light Curves of γ-ray Bursts. Astronomy & Astrophysics, 469, 379-385. 
https://doi.org/10.1051/0004-6361:20077530 
                
                
                    has been cited by the following article:
                
                
                    
                            - 
                                
                                    TITLE: 
                        
                            Swift XRT Analysis of Type II-P Supernova SN 2008ij
                                
                                
                                    AUTHORS: 
                                            SH. M. Shehata, Ahmed M. Fouad, R. M. Samir, A. A. Shaker 
                                                    
                                                        KEYWORDS: 
                        X-Ray Core Collapse Supernova, Swift (XRT) Observations 
                                                    
                                                    
                                                        JOURNAL NAME: 
                        International Journal of Astronomy and Astrophysics,  
                        Vol.14 No.3, 
                        September
                                                        10,
                        2024
                                                    
                                                    
                                                        ABSTRACT: This study investigates the X-ray properties and evolution of Type II supernovae (SNe II) observed by Swift, examining variations among supernovae and exploring their X-ray characteristics over time. We present the first X-ray study of the Type IIp supernova SN 2008ij using data from the Swift X-ray mission. This investigation focuses on its spectral properties, identifying an X-ray flux of 1.20 (+0.11, −0.10) × 10−13 erg/cm2/s and a plasma temperature of 4.76 (+1.22, −0.83) keV. Our study marks an advancement in understanding SN 2008ij, providing crucial results into its X-ray emission characteristics. These results lay the groundwork for future studies of Type IIp supernovae, offering a foundation for exploring their evolutionary and physical processes.