“…Such mirrors are inherently easier to grow, are less afflicted to detrimental roughening, hence allowing to obtain large Q-factors much easier than DBRs based on ternary AlGaAs alloys ; c) the substrate is transparent at the emission frequency, which makes transmission studies straight forward, being particularly appealing in resonant studies; d) compared to GaAs QWs, InGaAs QWs allow for a significantly higher flexibility in the design of the QW bandstructure. Consequently, the strain environment (hence the splitting between heavy hole and light holes), the emission wavelength, the oscillator strength and the tuning behavior in electric (via the quantum confined Stark effect) and magnetic fields can be conveniently adjusted via the QW thickness and the composition of the alloy [13][14][15][16]. In fact, it is possible to tune the wavelength band between 830 nm and 1200 nm, which is in particular appealing from the application point of view; e) InGaAs QWs have significantly larger exciton g-factors compared to GaAs/AlGaAs QWs [16], making them very interesting candidates to observe pronounced spinor polariton effects in a magnetic field [17].…”