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In the near future, the arrival of new surveys promises a significantincrement in the number of quasars (QSO) at large redshift ranges. This willhelp to constrain the dark energy models using quasars. The Large SynopticSurvey Telescope (LSST) will cover over 10 million QSO in six photometric bandsduring its 10-year run. QSO will be monitored and subsequently analysed usingthe photometric reverberation mapping technique. Oncoming LSST data willdecrease the uncertainties in the dark energy determination usingreverberating--mapped sources, particularly at high redshifts. We present thefirst steps in modelling of light curves for H$\beta$ and MgII and discuss thequasar selection in the context of photometric reverberation mapping with LSST.With the onset of the LSST era, we expect a huge rise in the overall quasarcounts and redshift range covered ($z\leq7.0$), which will provide a betterconstraint of AGN properties with cosmological purposes.

Generating AGN spectra for LSST: First steps