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20172022
most citedThe response of relativistic outflowing gas to the inner accretion disk of a black hole

146 citations · 816 across the 23 of their papers we have counts for

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Showing 2020Show all

14 papers · 1 filter

astro-ph.HE2020

Simultaneous NICER and NuSTAR Observations of the Ultra-compact X-ray Binary 4U 1543-624

R. M. Ludlam, A. D. Jaodand, J. A. García +8

We present the first joint NuSTAR and NICER observations of the ultra-compact X-ray binary (UCXB) 4U 1543624 obtained in 2020 April. The source was at a luminosity of $L_{0.5-50…

astro-ph.HE20206 cited

The Awakening Beast in the Seyfert 1 Galaxy KUG 1141+371 I

Jiachen Jiang, Huaqing Cheng, Luigi C. Gallo +10

KUG 1141+371 is a Seyfert 1 galaxy that shows a simultaneous flux increase in the optical and UV bands in the past decade. For instance, the latest Swift observation in 2019 shows…

astro-ph.HE202015 cited

MAXI J1820+070 with NuSTAR II. Flaring during the hard to soft state transition with a long soft lag

D. J. K. Buisson, A. C. Fabian, P. Gandhi +6

We continue the analysis of NuSTAR data from the recent discovery outburst of MAXI J1820+070 (optical counterpart ASASSN-18ey), focussing on an observation including unusual flarin…

astro-ph.HE2020

Discovery of thermonuclear (Type I) X-ray bursts in the X-ray binary Swift J1858.6-0814 observed with NICER and NuSTAR

D. J. K. Buisson, D. Altamirano, P. Bult +22

Swift J1858.6-0814 is a recently discovered X-ray binary notable for extremely strong variability (by factors in soft X-rays) in its discovery state. We present the detectio…

astro-ph.HE202047 cited

Measuring the masses of magnetic white dwarfs: A NuSTAR Legacy Survey

A. W. Shaw, C. O. Heinke, K. Mukai +11

The hard X-ray spectrum of magnetic cataclysmic variables can be modelled to provide a measurement of white dwarf mass. This method is complementary to radial velocity measurements…

astro-ph.HE202014 cited

Soft X-ray emission lines in the X-ray binary Swift J1858.6-0814 observed with XMM-Newton-RGS: disc atmosphere or wind?

D. J. K. Buisson, D. Altamirano, M. Díaz Trigo +11

We find soft X-ray emission lines from the X-ray binary Swift J1858.6-0814 in data from XMM-Newton-RGS: N VII, O VII and O VIII, as well as notable residuals short of a detection a…