The X-ray behaviour of the high-energy peaked BL Lacertae source PKS 2155−304 in the 0.3–10 keV band
Author:
Affiliation:
1. E. Kharadze Abastumani Astrophysical Observatory, Ilia State University, Tbilisi, GE-0162 Georgia
2. INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica, Via U. La Malfa 153, I-90146 Palermo, Italy
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/444/2/1077/24039821/stu1504.pdf
Reference76 articles.
1. THE SPECTRAL ENERGY DISTRIBUTION OFFERMIBRIGHT BLAZARS
2. VHEγ-ray emission of PKS 2155–304: spectral and temporal variability
3. A multiwavelength view of the flaring state of PKS 2155-304 in 2006
4. An intense soft high-latitude X-ray source H2156-304 - A new BL Lacertae object
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