Fig. 5
Simulations of various transient-type time series sampled every 1 day and with a Gaussian-distributed noise of 50 mmag (see text for more details). From top to bottom: a1) microlensing with an Einstein radius crossing time of 7.5 d, based on OGLE source SC4-267762; a2) microlensing with an Einstein radius crossing time of 153.5 d, based on OGLE source SC33-553617; b) nova event, based on V705 Cas; c1) and c2) dwarf nova events, based on sources OGLE-GD-DN-019 and OGLE-GD-DN-022, respectively; d) Be+neutron star system displaying recurrent bursts, based on source AX J0049.4-7323; e2) RCrB-type variability with intrinsic pulsations.
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