  The Vera Rubin Observatory will provide an unprecedented set of
time-dependent observations of the sky. The planned Legacy Survey of Space and
Time (LSST) operating for 10 years will provide dense lightcurves for thousands
of active galactic nuclei (AGN) in Deep Drilling Fields (DDFs) and less dense
lightcurves for millions of AGN. We model the prospects for measuring time
delays for emission lines with respect to the continuum, using these data. We
model the artificial lightcurves using Timmer-Koenig algorithm, we use the
exemplary cadence to sample them, we supplement lightcurves with the expected
contamination by the strong emission lines (Hbeta, Mg II and CIV as well as
with Fe II pseudo-continuum and the starlight). We choose the suitable
photometric bands appropriate for the redshift and compare the assumed line
time delay with the recovered time delay for 100 statistical realizations of
the light curves. We show that time delays for emission lines can be well
measured from the Main Survey for the bright tail of the quasar distribution
(about 15% of all sources) with the accuracy within 1 sigma error, for DDFs
results for fainter quasars are also reliable when all 10 years of data are
used. There are also some prospects to measure the time delays for the faintest
quasars at the smallest redshifts from the first two years of data, and
eventually even from the first season. The entire quasar population will allow
obtaining results of apparently high accuracy but in our simulations, we see a
systematic offset between the assumed and recovered time delay depending on the
redshift and source luminosity which will not disappear even in the case of
large statistics. Such a problem might affect the slope of the
radius-luminosity relation and cosmological applications of quasars if
simulations correcting for such effects are not performed.
