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 …

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 …

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 …

Here we present a detailed study of the broadband noise in the power density spectra of the
black hole X-ray binary MAXI J1820+ 070 during the hard state of its 2018 outburst, using …

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 …

Insight-HXMT is the first Chinese X-ray astronomical mission. With a 1–250 keV bandpass,
an energy resolution of 150 eV at 6 keV, and without being subject to pile-up distortions, it is …

We present a comprehensive spectral and temporal study of the black hole X-ray transient
MAXI J1820+ 070 during its outbursts in 2018 using Swift/XRT, NICER, NuSTAR, and …

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 …