activity
20062023
most citedMILES: A Medium resolution INT Library of Empirical Spectra

1.6k citations · 2k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.EP2023

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

Huan-Yu Teng, Bun'ei Sato, Masayuki Kuzuhara +15

In this study, we revisit 32 planetary systems around evolved stars observed within the framework of the Okayama Planet Search Program and its collaborative framework of the EAPS-N…

astro-ph.EP2022★ 23 cited

Detection of two additional circumbinary planets around Kepler-451

Ekrem Murat Esmer, Özgür Baştürk, Selim Osman Selam +1

We announce the detection of two new planetary-mass companions around Kepler-451 binary system in addition to the one detected previously based on eclipse timing variation analysis…

astro-ph.EP2021★ 3 cited

Analysis of the Most Precise Light Curves of HAT-P-36 Detrended From Spot Signals

Selçuk Yalçınkaya, Özgür Baştürk, Fadel El Helweh +6

We study the most precise light curves of the planet-host HAT-P-36 that we obtained from the ground primarily with a brand-new 80 cm telescope very recently installed at Ankara Uni…

astro-ph.SR2018

Starspot activity and differential rotation in KIC 11560447

Emre Isik, Ibrahim Ozavci, Hakan V. Senavci +4

Using high-precision photometry from the \textit{Kepler} mission, we investigate patterns of spot activity on the K1-type subgiant component of KIC 11560447, a short-period late-ty…

astro-ph.SR2017★ 29 cited

Recurrent starspot activity and differential rotation in KIC 11560447

İbrahim Özavci, Hakan V. Şenavci, Emre Işik +4

We present a detailed analysis of surface inhomogeneities on the K1-type sub-giant component of the rapidly rotating eclipsing binary KIC 11560447, using high-precision Kepler ligh…

astro-ph.SR2017★ 11 cited

A Jupiter-mass planet around the K0 giant HD 208897

M. Yılmaz, B. Sato, I. Bikmaev +9

For over 10 years, we have carried out a precise radial velocity (RV) survey to find substellar companions around evolved G,K-type stars to extend our knowledge of planet formation…