contributed to improve the first version of this manuscript. REM and JG acknowledge support by VRID-Enlace 216.016.002-1.0, BASAL Centro de Astrof[í]{}sica y Tecnolog[í]{}as Afines (CATA) PFB–06/2007 and FONDECYT 1190621. DS and REM thank FONDECYT 1201280 and DS thanks FONDECYT 1161247. JG acknowledges ANID project 21202285 and members of stellar variability group (S.V.G. UdeC) for useful discussions about this work. GD acknowledges the financial support of the Ministry of Education, Science and Technological Development of the Republic of Serbia through the contract No 451-03-68/2020/14/20002. The OGLE project has received funding from the Polish National Science Centre grant MAESTRO no. 2014/14/A/ST9/00121. This work has made use of data from the European Space Agency (ESA) mission [*Gaia*]{} (https://www.cosmos.esa.int/gaia), processed by the [*Gaia*]{} Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the [*Gaia*]{} Multilateral Agreement.

$$\begin{array}{llllllll}
            \hline
      %      \noalign{\smallskip}
{\rm Quantity} & {\rm OGLE-max}& {\rm Quantity}& {\rm OGLE-max} & {\rm Quantity} &{\rm OGLE-min} & {\rm Quantity}&{\rm OGLE-min}  \\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
   n                               & 142             & \cal M_{\rm_h} {[\cal M_{\odot}]} & 4.83  \pm 0.3 &    n                               & 85              & \cal M_{\rm_h} {[\cal M_{\odot}]} & 4.83  \pm 0.3 \\
{\rm \Sigma(O-C)^2}                