A long hard look at MCG-6-30-15 with XMM-Newton and BeppoSAX

Abstract

We summarise the primary results from a 320 ks observation of the bright Seyfert 1 galaxy MCG-6-30-15 with XMM-Newton and Beppo-SAX.

arXiv comment4 pages, 6 figures. Proc. of the meeting: "The Restless High-Energy Universe" (Amsterdam, The Netherlands), E.P.J. van den Heuvel, J.J.M. in 't Zand, and R.A.M.J. Wijers Eds

References in corpus (16)

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• The X-ray variability of the Seyfert~1 galaxy MCG-6-30-15 from long ASCA and RXTE observations
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• The continuum variability of MCG--6-30-15: A detailed analysis of the long 1999 ASCA observation
• The strength and width of Fe Kalpha lines in Seyferts and their correlations with the X-ray slope
• A two-component ionized reflection model of MCG--6-30-15
• The shape of the relativistic iron K-alpha line from MCG6--6-30-15 measured with the Chandra HETGS and RXTE

Cited by in corpus (4)

• Gravitating discs around black holes
• Reflection From the Strong Gravity Regime in a z=0.658 Gravitationally Lensed-Quasar
• Suzaku Discovery of a Hard Component Varying Independently of the Power-Law Emission in MCG-6-30-15
• Probing the origin of the iron K_alpha line around stellar and supermassive black holes using X-ray polarimetry