ner_tags: O B-Person O O O O O B-Organization I-Organization I-Organization O O O O O O B-Grant I-Grant I-Grant I-Grant I-Grant I-Grant B-Organization I-Organization I-Organization I-Organization O O B-Grant B-Person O O O B-Organization B-Person B-Person O B-Person O O O O B-Organization I-Organization I-Organization O O O O O O O O O B-Location B-Organization I-Organization I-Organization I-Organization O O B-Organization I-Organization I-Organization O O O O O O O O B-Telescope O O B-Organization O O O O O O O O O B-Organization O O O B-Organization O O O O O O B-Organization B-Telescope I-Telescope I-Telescope O O O O O B-Archive I-Archive I-Archive O O O O O O B-Organization I-Organization I-Organization I-Organization I-Organization O B-Organization I-Organization I-Organization I-Organization I-Organization B-Organization O O B-Organization I-Organization I-Organization I-Organization B-Organization O B-Telescope O O O O O B-Archive I-Archive I-Archive O O O O O O O O O O O B-Organization I-Organization I-Organization B-Organization O O O O B-Software O
tokens: ACKNOWLEDGEMENTS ZL thanks the support from the China Scholarship Council. This work is supported by the Strategic Pioneer Program on Space Science, Chinese Academy of Sciences, Grant No. XDA15052100. PTOB acknowledges support from STFC. JPO, PAE, and KLP acknowledge support from the UK Space Agency. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. This work is based on observation obtained with XMM–Newton , an ESA science mission with instruments and contributions directly fund by ESA Member States and NASA, based on observations made with the NASA/ESA Hubble Space Telescope , and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA) The Chandra data are obtained from the Chandra Data Archive . This research has made use of software provided by the Chandra X-ray Center (CXC) in the application packages ciao .