activity
20122024
most citedThe response of relativistic outflowing gas to the inner accretion disk of a black hole

146 citations · 1.2k across the 30 of their papers we have counts for

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Showing 2020Show all

14 papers · 1 filter

astro-ph.HE202039 cited

Extreme ultra-soft X-ray variability in an eROSITA observation of the Narrow-Line Seyfert 1 Galaxy 1H 0707-495

Th. Boller, T. Liu, P. Weber +9

The ultra-soft narrow-line Seyfert 1 galaxy 1H 0707-495 is a well-known and highly variable active galactic nucleus (AGN), with a complex, steep X-ray spectrum, and has been studie…

astro-ph.HE2020

Towards precision measurements of accreting black holes using X-ray reflection spectroscopy

Cosimo Bambi, Laura W. Brenneman, Thomas Dauser +14

Relativistic reflection features are commonly observed in the X-ray spectra of accreting black holes. In the presence of high quality data and with the correct astrophysical model,…

astro-ph.HE2020

The eROSITA X-ray telescope on SRG

P. Predehl, R. Andritschke, V. Arefiev +90

eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the primary instrument on the Spectrum-Roentgen-Gamma (SRG) mission, which was successfully launched on July 1…

astro-ph.HE2020

A variable ionized disk wind in the black-hole candidate EXO 1846-031

Yanan Wang, Long Ji, Javier A. Garcia +88

After 34 years, the black-hole candidate EXO 1846-031 went into outburst again in 2019. We investigate its spectral properties in the hard intermediate and the soft states with NuS…

astro-ph.HE202025 cited

A Full Characterisation of the Supermassive Black Hole in IRAS 09149-6206

D. J. Walton, W. N. Alston, P. Kosec +11

We present new broadband X-ray observations of the type-I Seyfert galaxy IRAS 09149-6206, taken in 2018 with -, and . The source is highly complex, sho…

astro-ph.HE2020

NuSTAR observation of GRO J1744-28 at low mass accretion rate

O. König, F. Fürst, P. Kretschmar +8

We present the spectral analysis of the LMXB GRO J1744-28 using 29 ks of NuSTAR data taken in 2017 February at a low luminosity of erg/s (3-50 keV). The c…