activity
20072026
most citedAbsolute properties of the binary system BB Pegasi

37 citations · 130 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.SR2026

Is the `Known' Enough? An Integrated Machine Learning Framework for Eclipsing Binary Classification and Parameter Estimation Based on Well-Characterized Systems

Burak Ulaş

This study presents a multi-task machine learning framework for simultaneous morphology classification and physical parameter estimation of eclipsing binaries using photometric lig…

astro-ph.SR2023

A Deep Learning Neural Network Algorithm for Classification of Eclipsing Binary Light Curves

Burak Ulas

We present an image classification algorithm using deep learning convolutional neural network architecture, which classifies the morphologies of eclipsing binary systems based on t…

astro-ph.SR2023

Six Newly Discovered Eclipsing Binary Systems in the TESS field

Burak Ulas, Vildan Ayan

We present the first detailed investigation of six eclipsing binary systems in the TESS field. The TESS light curves of the targets are analysed by determining the initial effectiv…

astro-ph.SR2022★ 2 cited

Discovery of Sct Components in Eclipsing Binary Systems IQ CMa, AW Men and W Vol

Burak Ulas, Ceren Ulusoy

We present the first evidence on the ~Sct type pulsations of the primary components of three eclipsing binaries IQ CMa, AW Men and W Vol in the TESS field. A comprehensive inves…

astro-ph.SR2022★ 3 cited

Discovery of pulsating components in eclipsing binary systems through the TESS light curves: The cases of CPD-30 740, HD 97329, V1637 Ori and TYC 683-640-1

Burak Ulaş, Ceren Ulusoy, Naci Erkan +2

We present the first evidence for the pulsations of primary components of four eclipsing binary systems. The TESS light curves of the targets are analyzed, the light and the absolu…

astro-ph.SR2021

Four New Eclipsing Binary Systems in the TESS field: CD-34 13220, HD 295082, TYC 6484-426-1 and TYC 6527-2310-1

Burak Ulas

We present the first evidence for the binarity of four targets in the TESS field. The temperatures are estimated by SED analysis and the orbital periods are determined. The TESS li…