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Presentation #215.03 in the session “Binary Stellar Systems I”.
We present new photometric data on the eclipsing binary LP133-373. Images were collected using two wide-band filters: Johnson V and Cousins R and were reduced using the Image Reduction and Analysis Facility (IRAF). All photometry was performed using the AstroImageJ(AIJ) software package and is multi-aperture differential photometry. Analysis includes the detection of a flare event and some eclipse timings. Previous studies by others have mentioned period changes and radial velocity changes over time, so we continue to monitor LP133-373.