We report optical photometric observations of the 2018 eruption (see ATels #12177, #12181, #12182, #12189, #12190, #12195, #12200, #12203, #12204) of the recurrent nova M31N 2008-12a (Henze et al. 2014, 2015a, 2015b,2018; Darnley et al. 2014, 2015, 2016). The data were obtained between 2018 Nov 06.0 UT - Nov 09.5 UT with the 0.96 m and 1.0 m SARA telescopes equipped with ARC CCD camera and Andor camera (Keel et al. 2017, located at the Kitt Peak National Observatory (SARA-KPNO), Arizona and Roque de los Muchachos, La Palma, Spain (SARA-ORM), respectively. The exposure times varied between 5 to 30 minutes. The derived magnitudes were calibrated with the standard stars in the field of this nova.
