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First X-ray spectrum of the most luminous quasar PKS 2126 - 158

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dc.contributor.author Ghosh, K. K
dc.contributor.author Soundararajaperumal, S
dc.date.accessioned 2008-06-17T05:13:07Z
dc.date.available 2008-06-17T05:13:07Z
dc.date.issued 1992-11
dc.identifier.citation A&A, Vol. 265, pp. 413 - 416 en
dc.identifier.uri http://hdl.handle.net/2248/2438
dc.description.abstract For the first time the detailed results of the spectral analysis of the X-ray (0.1 - 10 keV) spectrum of the luminous radio-loud quasar PKS 2126 - 158 are presented. Power law and fixed absorption model fits well with the spectrum. The parameters of this model suggest that this quasar is a flat spectrum source. Derived soft (0.1 - 2 keV) and hard (2 - 10 keV) X-ray luminosities of this quasar are (0.7 +/- 0.1) 10 exp 48 erg/s and (2.3 +/- 0.3) 10 exp 48 erg/s, respectively. No soft excess and low energy absorption have been detected in this source. Thermal bremsstrahlung model also fits well with the spectrum of PKS 2126 - 158 and the derived rest-frame temperature is 6.4 + 40 or -4 keV. This is the most luminous quasar which has been detected in the hard X-rays en
dc.format.extent 506738 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher EDP Sciences en
dc.relation.uri http://adsabs.harvard.edu/abs/1992A%26A...265..413G en
dc.subject LUMINOSITY en
dc.subject QUASARS, X RAY SPECTRA en
dc.subject ASTRONOMICAL MODELS en
dc.subject EXOSAT SATELLITE en
dc.subject SPECTRUM ANALYSIS en
dc.title First X-ray spectrum of the most luminous quasar PKS 2126 - 158 en
dc.type Article en


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