activity
20192026
most citedInvestigation of the Orbital Period and Mass Relations for W UMa-type Contact Systems

39 citations · 179 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.EP2026

Two temperate Earth- and Neptune-sized planets orbiting fully convective M dwarfs

Madison G. Scott, Georgina Dransfield, Mathilde Timmermans +30

As the diversity of exoplanets continues to grow, it is important to revisit assumptions about habitability and classical HZ definitions. In this work, we introduce an expanded 'te…

astro-ph.EP2025★ 8 cited

Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267

S. Zúñiga-Fernández, F. J. Pozuelos, M. Dévora-Pajares +63

We report two warm Earth-sized exoplanets orbiting the close binary TOI-2267 (M5+M6, separation ~8 au). Data from TESS and ground-based facilities confirm the planets, but we canno…

astro-ph.IM2025★ 2 cited

SPECULOOS: five years hunting terrestrial planets around ultra-cool dwarfs

Sebastián Zúñiga-Fernández, Michael Gillon, SPECULOOS consortium

The SPECULOOS (Search for habitable Planets EClipsing ULtra-cOOl Stars) project aims to detect temperate terrestrial planets transiting nearby ultracool dwarfs, including late M-dw…

astro-ph.EP2025

Gravity-sensitive Spectral Indices in Ultracool Dwarfs: Investigating Correlations with Metallicity and Planet Occurrence using SpeX and FIRE Observations

Fatemeh Davoudi, Benjamin V. Rackham, Julien de Wit +5

We present a near-infrared spectroscopic analysis (0.9--2.4~m) of gravity indices for 56 ultracool dwarfs (M5.5--L0), including exoplanet hosts SPECULOOS-2, SPECULOOS-3, and LHS…

astro-ph.EP2025

TOI-6508b: A massive transiting brown dwarf orbiting a low-mass star

K. Barkaoui, D. Sebastian, S. Zúñiga-Fernández +44

We report the discovery of a transiting brown dwarf orbiting a low-mass star, TOI-6508b. Today, only ~50 transiting brown dwarfs have been discovered. TOI-6508b was first detected…

astro-ph.EP2025

TOI-2015b: a sub-Neptune in strong gravitational interaction with an outer non-transiting planet

K. Barkaoui, J. Korth, E. Gaidos +119

TOI-2015 is a known exoplanetary system around an M4 dwarf star, consisting of a transiting sub-Neptune planet in a 3.35-day orbital period, TOI-2015b, accompanied by a non-transit…

astro-ph.EP2024★ 11 cited

TESS discovery of two super-Earths orbiting the M-dwarf stars TOI-6002 and TOI-5713 near the radius valley

M. Ghachoui, B. V. Rackham, M. Dévora-Pajares +45

We present the validation of two TESS super-Earth candidates transiting the mid-M dwarfs TOI-6002 and TOI-5713 every 10.90 and 10.44 days, respectively. The first star (TOI-6002) i…

astro-ph.EP2024★ 8 cited

TOI-4336 A b: A temperate sub-Neptune ripe for atmospheric characterization in a nearby triple M-dwarf system

M. Timmermans, G. Dransfield, M. Gillon +54

Small planets transiting bright nearby stars are essential to our understanding of the formation and evolution of exoplanetary systems. However, few constitute prime targets for at…

astro-ph.EP2024★ 10 cited

Looking For Timing Variations in the Transits of 16 Exoplanets

S. Yalçınkaya, E. M. Esmer, Ö. Baştürk +27

We update the ephemerides of 16 transiting exoplanets using our ground-based observations, new TESS data, and previously published observations including those of amateur astronome…

astro-ph.EP2023

TOI-2084 b and TOI-4184 b: two new sub-Neptunes around M dwarf stars

K. Barkaoui, M. Timmermans, A. Soubkiou +67

We present the discovery and validation of two TESS exoplanets orbiting nearby M dwarfs: TOI-2084b, and TOI-4184b. We characterized the host stars by combining spectra from Shane/K…

astro-ph.SR2022

The Photometric Study of Six W UMa Systems and Investigation of the Mass-Radius Relations for Contact Binary Stars

Atila Poro, Ehsan Paki, Mark G. Blackford +13

We present the photometric analysis of six short-period systems (EI Oct, V336 TrA, NX Boo, V356 Boo, PS Boo, and V2282 Cyg). This is the first photometric analysis of these systems…

astro-ph.EP2022★ 16 cited

Homogeneous Transit Timing Analyses of Ten Exoplanet Systems

Ö. Baştürk, E. M. Esmer, S. Yalçınkaya +19

We study the transit timings of 10 exoplanets in order to investigate potential Transit Timing Variations (TTVs) in them. We model their available ground-based light curves, some p…

astro-ph.SR2021★ 39 cited

Investigation of the Orbital Period and Mass Relations for W UMa-type Contact Systems

Atila Poro, Soroush Sarabi, Shiva Zamanpour +14

New relationships between the orbital period and some parameters of W Ursae Majoris (W UMa) type systems are presented in this study. To investigate the relationships, we calculate…

astro-ph.EP2021★ 18 cited

Investigation of an orbital decay and global modeling of the planet WASP-43 b

Fatemeh Davoudi, Özgür Baştürk, Selçuk Yalçınkaya +2

WASP-43 b is one of the most important candidates for detecting an orbital decay. We investigate pieces of evidence for this expectation as variations in its transit timings, based…

astro-ph.SR2021

The New Ephemeris and Light Curve Analysis of V870 Ara by the Ground-Based and TESS Data

Atila Poro, Mark G. Blackford, Fatemeh Davoudi +4

New CCD photometric observations and their investigation of the W UMa-type binary, V870 Ara, are presented. Light curves of the system were taken through BVI filters from the Conga…

astro-ph.SR2021★ 27 cited

Observational and Theoretical Studies of 27 Scuti Stars with Investigation of the Period-Luminosity Relation

Atila Poro, Ehsan Paki, Golnaz Mazhari +11

The multi-color CCD photometric study of 27 Delta Scuti stars is presented. By using approximately three years of photometric observations, we obtained the times of maxima and magn…

astro-ph.EP2020★ 4 cited

Refined Ephemeris for Four Hot Jupiters using Ground-Based and TESS Observations

Fatemeh Davoudi, PegahSadat MirshafieKhozani, Ehsan Paki +11

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 by the T…

astro-ph.SR2020★ 1 cited

The First Light Curve Solutions of GW Leo and Period Study of Two Contact Binary Systems

Atila Poro, Afshin Halavati, Elahe Lashgari +5

We performed the first light curve analysis of GW Leo and a new ephemeris is obtained for QT Boo. In the present photometric study of two contact binary systems, we found that the…

astro-ph.SR2020

BVRI Photometric Observations, Light Curve Solutions and Orbital Period Analysis of BF Pav

Atila Poro, Fahri Alicavus, Eduardo Fernández-Lajús +7

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 fil…

astro-ph.SR2020★ 3 cited

The First Light Curve Solutions and Period Changes of EW Psc and HN Psc

F. Davoudi, A. Poro, F. Alicavus +13

The first light curve solutions of the stars EW and HN in Pisces constellation are presented. Photometry, and its' periodic changes are calculated and discussed. The analysis of O-…

astro-ph.EP2020

Radius Study of Ten Transiting Hot Jupiter Exoplanets with Ground-Based Observations

F. Davoudi, A. Poro, E. Paki +9

In this research, 14 light curves of 10 hot Jupiter exoplanets available on Exoplanet Transit Database (ETD) were analyzed. We extracted the transit parameters using EXOFAST softwa…

astro-ph.SR2020★ 15 cited

The First Light Curve Solutions and Period Study of BQ Ari

A. Poro, F. Davoudi, F. Alicavus +14

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 (W-D)…

astro-ph.EP2019★ 2 cited

Transit Timing Variations of Five Transiting Planets

Ozgur Basturk, Ekrem M. Esmer, Seyma Torun +10

Transiting planets provide a unique opportunity to search for unseen additional bodies gravitationally bound to a system. It is possible to detect the motion of the center-of-mass…

astro-ph.EP2019★ 15 cited

Light Curve Analysis of Ground-Based Data from Exoplanets Transit Database

F. Davoudi, S. J. Jafarzadeh, A. Poro +9

Photometric observations of exoplanet transits can be used to derive the orbital and physical parameters of an exoplanet. We analyzed several transit light curves of exoplanets tha…