MAXI J1348–630 is a low mass X-ray binary discovered in 2019 during a bright outburst.
During this event, the system experienced both hard and soft states following the standard …

Black hole (BH) X-ray binaries (XRBs) are ideal targets to study the connection between
accretion inflow and jet outflow. Here we present quasi-simultaneous, multiwavelength …

The black hole X-ray transient MAXI J1820+ 070 (= ASSASN-18ey) discovered in 2018
March was one of the optically brightest ever seen, which has resulted in very detailed …

The recurring transient outbursts in low-mass X-ray binaries (LMXBs) provide ideal
laboratories to study the accretion process. Unlike their supermassive relatives, LMXBs are …

We present optical monitoring of the neutron star low-mass X-ray binary Swift J1858. 6–
0814 during its 2018–2020 outburst and subsequent quiescence. We find that there was …

ABSTRACT Centaurus X–4 (Cen X–4) is a relatively nearby neutron star low-mass X-ray
binary that showed outbursts in 1969 and 1979, but has not shown a full outburst since. Due …

Abstract We present long-term (2012–2022) optical monitoring of the candidate black hole X-
ray binary Swift J1910. 2–0546 with the Faulkes Telescopes and Las Cumbres Observatory …

Abstract The Einstein Probe (EP) is an interdisciplinary mission of time-domain and X-ray
astronomy. Equipped with a wide-field lobster-eye X-ray focusing imager, EP will discover …

Context. It is now widely accepted that most ultraluminous X-ray sources (ULXs) are binary
systems whose large (above 10 39 erg s− 1) apparent luminosities are explained by super …

A Multiwavelength Study of GRS 1716-249 in Outburst: Constraints on Its System
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