The launch of NuSTAR and the increasing number of binary black hole (BBH) mergers
detected through gravitational wave observations have exponentially advanced our …

We report the X-ray timing results of the black hole candidate MAXI J1820+ 070 during its
2018 outburst using the Hard X-ray Modulation Telescope (Insight-HXMT) and Neutron Star …

The optical emission line spectra of X-ray binaries (XRBs) are thought to be produced in an
irradiated atmosphere, possibly the base of a wind, located above the outer accretion disc …

Accreting black hole binaries change their properties during evolution, passing through two
main luminous states, dominated by either hard or soft X-rays. In the hard state, steady …

Although low-frequency quasiperiodic oscillations (LFQPOs) are commonly detected in the
X-ray light curves of accreting black hole X-ray binaries, their origin still remains elusive. In …

We analyse the X-ray spectrum of the black hole (BH) X-ray binary MAXI J1820+ 070 using
observations from XMM-Newton and NuSTAR during 'hard'states of its 2018–2019 outburst …

ABSTRACT MAXI J1348− 630 is a low-mass X-ray black hole binary located in the Galaxy
and undergone the X-ray outburst in 2019. We analysed the observation data in very soft …

ABSTRACT MAXI J1820+ 070 (ASSASN-18ey) is a black hole (BH) X-ray binary discovered
in 2018. The brightness of the source triggered multi-wavelength campaigns of this source …

We report results on the joint-fit of the NuSTAR and HXMT data for the black hole X-ray
binary candidate MAXI J1535-571. The observations were obtained in 2017 when the …

The black hole X-ray binary source 4U 1543–47 experienced a super-Eddington outburst in
2021, reaching a peak flux of up to∼ 1.96× 10− 7 erg cm− 2 s− 1 (∼ 8.2 Crab) in the 2− 10 …