activity
20072026
most citedTriple-Star Candidates Among the Kepler Binaries

173 citations · 588 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2026

Photometric Modulations on Intermediate Timescales in the Symbiotic Binaries

Melis Yardımcı, Samet Ok, Belinda Kalomeni

We present a multi-band study of three symbiotic binaries using combined ground- and space-based monitoring that spans up to 14 years. These datasets enable a systematic investigat…

astro-ph.SR2026

A Binary-Based Reassessment of the Age and Stellar Properties of NGC 7789 Using Twelve Binary Components

Kadri Yakut, Belinda Kalomeni, Saul Rappaport

We present a binary-based reassessment of the age of the intermediate-age open cluster NGC 7789, together with well-constrained stellar parameters for twelve components in six SB2…

astro-ph.SR2025

A Deep Look into the Intermediate-Age Open Cluster NGC 2506: What Binary Systems Reveal About Cluster Distance and Age

K. Yakut, B. Kalomeni, S. Rappaport +1

Using high-precision observations from the space-based \textit{Gaia} and \textit{TESS} missions, complemented by ground-based spectroscopic data and multi-band photometric surveys,…

astro-ph.SR2025

A novel approach to determining the age of stellar clusters: application to NGC 188

K. Yakut, B. Kalomeni, S. Rappaport

We present a new independent determination for the age of one of the oldest open clusters, NGC 188: Gyr. We utilize a novel approach where we jointly fit the radial…

astro-ph.SR2025

Comprehensive analysis of CM Draconis: eclipse timing variations driven by either a third body or stellar magnetic activity

B. Kalomeni, K. Yakut

The CM Draconis system is a well-studied, double-lined spectroscopic binary that is totally eclipsing and exhibits strong magnetic activity. Nearly one million photometric measurem…

astro-ph.HE2021★ 8 cited

Light curve properties of SN 2017fgc and HV SNe Ia

Umut Burgaz, Keiichi Maeda, Belinda Kalomeni +5

Photometric and spectroscopic observations of type Ia supernova (SN) 2017fgc which cover the period from 12 to +137 days since the -band maximum are presented. SN 2017fgc is…