activity
19952014
most citedAn Explanation for the soft X-ray excess in AGN

479 citations · 2.8k across the 30 of their papers we have counts for

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Showing 2002Show all

5 papers · 1 filter

astro-ph2002★ 44 cited

Multiple X-ray reflection from ionized slabs

R. R. Ross, A. C. Fabian, D. R. Ballantyne

Multiple reflection of X-rays may be important when an accretion disc and its hot corona have a complicated geometry, or if returning radiation due to gravitational light bending i…

astro-ph2002

Reflection Spectra from Photoionized Accretion Discs

D. R. Ballantyne, R. R. Ross, A. C. Fabian

We review recent progress on the modeling and use of reflection spectra from irradiated and ionized accretion discs. On the computational side, calculations of reflection spectra f…

astro-ph2002★ 46 cited

Soft X-ray emission lines from photoionized accretion discs: constraints on their strength and width

D. R. Ballantyne, R. R. Ross, A. C. Fabian

We consider the properties of soft X-ray emission lines in the reprocessed emission from a photoionized accretion disc. Observations of these lines will be important in determining…

astro-ph2002★ 29 cited

The response of the Fe Kαline to changes in the X-ray illumination of accretion discs

D. R. Ballantyne, R. R. Ross

X-ray reflection spectra from photoionized accretion discs in active galaxies are presented for a wide range of illumination conditions. The energy, equivalent width (EW) and flux…

astro-ph2002★ 41 cited

On the hard X-ray spectra of radio-loud active galaxies

D. R. Ballantyne, R. R. Ross, A. C. Fabian

Over the last few years X-ray observations of broad-line radio galaxies (BLRGs) by ASCA, RXTE and BeppoSAX have shown that these objects seem to exhibit weaker X-ray reflection fea…