nearby active galaxy M87. Since the typical timescale of an AGN or a microquasar scales with mass, temporal behaviour of black hole candidates is studied with microquasars [@mkkf06]. After investigating the connection between accretion and ejection in ten microquasars, @gfp03 concluded that mildly relativistic, quasi steady jets are generally ejected in the low hard spectral states (when electromagnetic spectra peak in the high energy power-law frequency range) of the accretion disc. It was also shown that jets tend to get stronger as the microquasar moves to the intermediate hard states, and truly relativistic ejections are observed during hard-intermediate to soft-intermediate transition, after which the microquasar enters canonical high soft state (when spectra peak in the thermal low energy range), which shows no jet activity [@rsfp10; @mil12]. All these evidences suggest that the generation or quenching of jets do depend on various states of the accretion disc, and that, the jet formation mechanism is linked with the processes that dominate at distances relatively closer to the black hole.

It is well known that, spectra from microquasar change states between, the low hard state (LH) and high soft state (HS), through a series of intermediate states. Interestingly, the hard power-law photons exhibit 