activity
20082026
most citedDetermining the covering factor of Compton-thick active galactic nuclei with NuSTAR

82 citations · 1.1k across the 53 of their papers we have counts for

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Showing 2019Show all

16 papers · 1 filter

astro-ph.HE2019

Swift monitoring of M51: A 38-day super-orbital period for the pulsar ULX7 and a new transient ULX

Murray Brightman, Hannah Earnshaw, Felix Fürst +6

We present the results from a monitoring campaign made with the Neil Gehrels Swift Observatory of the M51 galaxies, which contain several variable ultraluminous X-ray sources (ULXs…

astro-ph.HE2019★ 24 cited

Discovery of a soft X-ray lag in the Ultraluminous X-ray Source NGC 1313 X-1

E. Kara, C. Pinto, D. J. Walton +14

Ultraluminous X-ray Sources (ULXs) provide a unique opportunities to probe the geometry and energetics of super-Eddington accretion. The radiative processes involved in super-Eddin…

astro-ph.HE2019★ 5 cited

The Broadband X-ray Spectrum of the X-ray Obscured Type 1 AGN 2MASX J193013.80+341049.5

Nikita Kamraj, Mislav Baloković, Murray Brightman +6

We present results from modeling the broadband X-ray spectrum of the Type 1 AGN 2MASX J193013.80+341049.5 using NuSTAR, Swift and archival XMM-Newton observations. We find this sou…

astro-ph.HE2019

The Unusual Broadband X-ray Spectral Variability of NGC 1313 X-1 seen with XMMNewton, Chandra and NuSTAR

D. J. Walton, C. Pinto, M. Nowak +19

We present results from the major coordinated X-ray observing program on the ULX NGC 1313 X-1 performed in 2017, combining -, and , focusing on the e…

astro-ph.HE2019

Discovery of a red supergiant donor star in SN2010da/NGC 300 ULX-1

M. Heida, R. M. Lau, B. Davies +7

SN2010da/NGC 300 ULX-1 was first detected as a supernova impostor in May 2010 and was recently discovered to be a pulsating ultraluminous X-ray source. In this letter, we present V…

astro-ph.HE2019

X-ray spectral and eclipsing model of the clumpy obscurer in active galactic nuclei

Johannes Buchner, Murray Brightman, Kirpal Nandra +2

We present a unification model for a clumpy obscurer in active galactic nuclei (AGN) and investigate the properties of the resulting X-ray spectrum. Our model is constructed to rep…