activity
20102022
most citedAsymmetric transit curves as indication of orbital obliquity: clues from the late-type dwarf companion in KOI-13

136 citations · 437 across the 16 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2022★ 18 cited

Variable star classification with a Multiple-Input Neural Network

T. Szklenár, A. Bódi, D. Tarczay-Nehéz +3

In this experiment, we created a Multiple-Input Neural Network, consisting of Convolutional and Multi-layer Neural Networks. With this setup the selected highest-performing neural…

astro-ph.SR2020★ 23 cited

Image-based Classification of Variable Stars: First Results from Optical Gravitational Lensing Experiment Data

T. Szklenár, A. Bódi, D. Tarczay-Nehéz +5

Recently, machine learning methods presented a viable solution for automated classification of image-based data in various research fields and business applications. Scientists req…

astro-ph.SR2017★ 25 cited

An UXor among FUors: extinction related brightness variations of the young eruptive star V582 Aur

P. Ábrahám, Á. Kóspál, M. Kun +24

V582 Aur is an FU Ori-type young eruptive star in outburst since 1985. The eruption is currently in a relatively constant plateau phase, with photometric and spectroscopic va…

astro-ph.SR2014★ 5 cited

Discovery of the spectroscopic binary nature of the classical Cepheids FN Aql and V1344 Aql

L. Szabados, B. Cseh, J. Kovács +8

We present the analysis of photometric and spectroscopic data of two classical Cepheids, FN Aquilae and V1344 Aquilae. Based on the joint treatment of the new and earlier radial ve…

astro-ph.SR2012★ 110 cited

HD 181068: A Red Giant in a Triply-Eclipsing Compact Hierarchical Triple System

A. Derekas, L. L. Kiss, T. Borkovits +41

Hierarchical triple systems comprise a close binary and a more distant component. They are important for testing theories of star formation and of stellar evolution in the presence…

astro-ph.SR2011★ 28 cited

Inner disc rearrangement revealed by dramatic brightness variations in the young star PV Cep

M. Kun, E. Szegedi-Elek, A. Moór +11

Young Sun-like stars at the beginning of the pre-main sequence (PMS) evolution are surrounded by accretion discs and remnant protostellar envelopes. Photometric and spectroscopic v…