most citedThe Soft State of the Black Hole Transient Source MAXI J1820+070: Emission from the Edge of the Plunge Region?

67 citations · 297 across the 9 of their papers we have counts for

collaborators

9 papers

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…

astro-ph.HE202023 cited

X-ray Spectral and Timing evolution of MAXI J1727-203 with NICER

K. Alabarta, D. Altamirano, M. Méndez +16

We present a detailed X-ray spectral and variability study of the full 2018 outburst of MAXI J1727-203 using NICER observations. The outburst lasted approximately four months. Spec…

astro-ph.HE202039 cited

A NICER look at the state transitions of the black hole candidate MAXI J1535-571 during its reflares

V. A. Cúneo, K. Alabarta, L. Zhang +18

The black hole candidate and X-ray binary MAXI J1535-571 was discovered in September 2017. During the decay of its discovery outburst, and before returning to quiescence, the sourc…

astro-ph.HE202022 cited

The variable radio counterpart of Swift J1858.6-0814

J. van den Eijnden, N. Degenaar, T. D. Russell +18

Swift J1858.6-0814 is a transient neutron star X-ray binary discovered in October 2018. Multi-wavelength follow-up observations across the electromagnetic spectrum revealed many in…

astro-ph.HE202067 cited

The Soft State of the Black Hole Transient Source MAXI J1820+070: Emission from the Edge of the Plunge Region?

A. C. Fabian, D. J Buisson, P. Kosec +18

The Galactic black hole X-ray binary MAXI J1820+070 had a bright outburst in 2018 when it became the second brightest X-ray source in the Sky. It was too bright for X-ray CCD instr…