activity
20002018
most citedMethods for exomoon characterisation: combining transit photometry and the Rossiter-McLaughlin effect

60 citations · 208 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2018★ 23 cited

The contact binary VW Cephei revisited: surface activity and period variation

T. Mitnyan, A. Bódi, T. Szalai +7

Context. Despite the fact that VW Cephei is one of the well-studied contact binaries in the literature, there is no fully consistent model available that can explain every observed…

astro-ph.SR2016★ 20 cited

Periodicities of the RV Tau-type pulsating star DF Cygni: a combination of Kepler data with ground-based observations

A. Bódi, K. Szatmáry, L. L. Kiss

The RV Tauri stars constitute a small group of classical pulsating stars with some dozen known members in the Milky Way. The light variation is caused predominantly by pulsations,…

astro-ph.SR2013★ 44 cited

Variability of M giant stars based on Kepler photometry: general characteristics

E. Bányai, L. L. Kiss, T. R. Bedding +15

M giants are among the longest-period pulsating stars which is why their studies were traditionally restricted to analyses of low-precision visual observations, and more recently,…

astro-ph.SR2010★ 60 cited

Methods for exomoon characterisation: combining transit photometry and the Rossiter-McLaughlin effect

A. E. Simon, Gy. M. Szabó, K. Szatmáry +1

It has been suggested that moons around transiting exoplanets may cause observable signal in transit photometry or in the Rossiter-McLaughlin (RM) effect. In this paper a detailed…

astro-ph2002★ 30 cited

The Type la Supernova 2001V in NGC 3987

J. Vinko, I. B. Biro, B. Csak +10

CCD photometry of the type Ia SN 2001V occured in the edge-on spiral galaxy NGC 3987 is presented. The observations made through Johnson-Cousins BVRI filters were collected from Fe…

astro-ph2000★ 31 cited

Multiperiodicity in semiregular variables II. Systematic amplitude variations

L. L. Kiss, K. Szatmary, Gy. Szabo +1

We present a detailed lightcurve analysis for a sample of bright semiregular variables based on long-term (70--90 years) visual magnitude estimates carried out by amateur astronome…