Light curve modeling of the two short period eclipsing binaries ATO J009.3383 + 34.2329 and CRTS J004004.7 + 385531

Abstract

In this study, we present a detailed photometric analysis of two short-period eclipsing binary systems, ATOJ009.3383 + 34.2329 and CRTSJ004004.7 + 385531. The photometric data for our analysis was obtained from the Zwicky Transient Facility (ZTF) catalogue at gri filters and the Transiting Exoplanet Survey Satellite (TESS) database. Based on our analysis, we classify both systems as W Uma-type binaries, with A-subtype. To estimate the physical and geometrical parameters of these systems, we employ the PHEOBE code. This results in two totally eclipsing systems with degree of inclination (i) of around 68 and 88 deg, respectively. The ATOJ009.3383 + 34.2329 indicates a low mass ratio (q) binary with q = 0.107, while CRTSJ004004.7 + 385531 exhibits a moderate q value of 0.545. A cool spot on the surface of the secondary star of CRTSJ004004.7 + 385531 with a 30% cooler atmosphere of the surrounding surface is detected. This is explained by magnetic activity on the surface of CRTSJ004004.7 + 385531. Our findings reveal overcontact fill-out factor f with 54 and 52% for ATOJ009.3383 + 34.2329 and CRTSJ004004.7 + 385531, respectively. In addition to the light curve modeling, we calculate new epochs and ephemeris for both binary systems. The absolute parameters for the two systems are estimated. Eventually, the systems’ evolutionary status along ZAMS and TAMS are discussed.