activity
20182021
most citedSearching for Ultra-fast Outflows in AGN using Variability Spectra

60 citations · 122 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.HE202111 cited

Discovery of soft and hard X-ray time lags in low-mass AGNs

Labani Mallick, Daniel R. Wilkins, William N. Alston +5

The scaling relations between the black hole (BH) mass and soft lag properties for both active galactic nuclei (AGNs) and BH X-ray binaries (BHXRBs) suggest the same underlying phy…

astro-ph.HE20206 cited

Modelling X-ray RMS spectra II: the ultra-fast outflow of PDS 456

L. Härer, M. L. Parker, A. Joyce +6

We present an improved model for excess variance spectra describing ultra-fast outflows and successfully apply it to the luminous (L ~ 10^47 erg/s) low-redshift (z = 0.184) quasar…

astro-ph.HE202020 cited

Detection of a variable ultra-fast outflow in the Narrow Line Seyfert 1 galaxy PG 1448+273

P. Kosec, A. Zoghbi, D. J. Walton +4

Relativistically blueshifted absorption features of highly ionised ions, the so-called ultra-fast outflows (UFOs), have been detected in the X-ray spectra of a number of accreting…

astro-ph.HE202060 cited

Searching for Ultra-fast Outflows in AGN using Variability Spectra

Z. Igo, M. L. Parker, G. A. Matzeu +8

We present a qualitative search for ultra-fast outflows (UFOs) in excess variance spectra of radio-quiet active galactic nuclei (AGN). We analyse 42 sources from the Tombesi et al.…

astro-ph.HE201925 cited

Modelling X-ray RMS spectra I: intrinsically variable AGN

M. L. Parker, W. N. Alston, Z. Igo +1

We present simple XSPEC models for fitting excess variance spectra of AGN. Using a simple Monte-Carlo approach, we simulate a range of spectra corresponding to physical parameters…

astro-ph.HE2018

Relativistic spectroscopy of the extreme NLS1 IRAS13224-3809

M. L. Parker, W. N. Alston, D. J. K Buisson +5

The narrow line Seyfert 1 (NLS1) IRAS 13224-3809 is the most X-ray variable active galactic nucleus (AGN), exhibiting 0.3-10 keV flux changes of over an order of magnitude within a…