High-precision transit photometry supplies ideal opportunities for detecting new exoplanets
and characterizing their physical properties, which usually encode valuable information for …

The first analysis of the photometric observation in BVR filters of a W UMa type binary
system BQ Ari was performed. Light curve analysis was performed using Wilson–Devinney …

Scientific-grade cameras are frequently employed in industries such as spectral imaging
technology, aircraft, medical detection, and astronomy, and are characterized by high …

High-precision transit observations provide excellent opportunities for characterizing the
physical properties of exoplanetary systems. These physical properties supply many pieces …

New observations of the eclipsing binary system V1848 Ori were carried out using the V filter
resulting in a determination of new times of minima and new ephemeris were obtained. We …

A new ephemeris, period change analysis and light curve modeling of the W UMa-type
eclipsing binary BF Pav are presented in this study. Light curves of the system taken in BVRI …

Exoplanets are celestial bodies orbiting stars beyond our Solar System. Although historically
they posed detection challenges, Kepler's data has revolutionized our understanding. By …

Abstract WASP-12 b, WASP-33 b, WASP-36 b, and WASP-46 b are four transiting hot
Jupiters, which we have studied. These systems' light curves were derived from …

From the light curve taken during exoplanet transit, important parameters such as the radius
ratio of the star-planet, impact parameter, inclination, and relative tangential velocity could …

WASP-12 b, WASP-33 b, WASP-36 b, and WASP-46 b are four transiting planetary systems
which we have studied. These systems' light curves were derived from observations made …